The galaxy presents as a slightly elongated, disk-like structure oriented at an angle relative to the observer, with the major axis appearing to be tilted from our perspective. The central region exhibits a concentrated, bright luminosity suggesting a high density of stars, possibly an active galactic nucleus or a significant stellar bulge. 

Moving outwards from the center, the galaxy appears to transition into a less defined disk, with subtle hints of spiral arm structures. Color gradients are observed, with the central regions showing redder hues, potentially indicating an older stellar population, and bluer tones in the outer regions, which could indicate ongoing star formation activity.

The galaxy displays some irregular features, possibly signs of minor disturbances or interactions. The overall appearance suggests a system that has experienced some level of dynamical evolution, possibly through past mergers or tidal interactions. The light distribution across the galaxy is relatively smooth, but hints of clumpy regions suggest areas of active star formation or unresolved stellar groupings.
