The galaxy appears as a somewhat elliptical, though not perfectly round, structure. The central region exhibits a bright, concentrated luminosity, suggestive of a significant stellar population or possibly an active galactic nucleus. Moving outwards from the core, the luminosity decreases.

A distinct, slightly bluer region is observed to the left of the galaxy's center. This may indicate a region of active star formation, characterized by the presence of younger, hotter stars.

Overall, the galaxy presents a relatively smooth appearance, but there are hints of some disturbed morphologies, possibly tidal tails. The color gradients suggest variations in stellar populations and dust content across the galaxy. The galaxy seems to have an intermediate mass and star formation rate.
