The galaxy appears as a centrally concentrated object with a largely smooth morphology, indicative of an elliptical galaxy or a spiral galaxy seen face-on with a prominent bulge. The central region exhibits a higher surface brightness, while the outer regions gradually fade, suggesting a decline in stellar density with increasing radial distance. The color profile is relatively uniform across the galaxy, with a slight tendency towards redder hues in the center and bluer hues toward the edges, possibly suggesting the presence of younger stars or ongoing star formation in the outer regions. Faint, disturbed features might be present in the galaxy's outskirts, warranting closer inspection. There does not appear to be a prominent disk-like structure, strong spiral arms, or significant dust lanes. The overall impression is that of a mature galaxy with moderate star formation activity.
