The galaxy presents as a somewhat elongated structure, with an apparent major axis longer than its minor axis, suggesting an elliptical or possibly a spiral galaxy viewed at an angle. The central region exhibits a concentrated luminosity, indicative of a dense stellar population, possibly a bulge. The color of this central region appears to be yellow-ish, suggesting an older stellar population. Moving outwards from the center, there's a transition to bluer hues in the outer regions, particularly noticeable at the edges. This suggests the presence of younger, hotter stars and ongoing star formation in the galactic disk. There is no obvious spiral structure visible, but there is some visual evidence of disturbance or asymmetry. Overall, the galaxy appears to be a relatively massive system with a mix of stellar populations.
