The galaxy presents an elongated morphology, suggesting a possible disk-like structure viewed at an angle. The central region appears bright and yellowish-white, indicative of an older stellar population and possibly a bulge component. Moving outwards from the center, there's a transition to a bluer hue, particularly noticeable on one side of the galaxy. This bluer region likely indicates ongoing star formation activity, traced by younger, hotter stars. A distinct, reddish region is observed at the upper part of the galaxy. It's likely either a region of dust obscuration, or a region of intense star formation, where light from stars is reddened by dust. Overall, the galaxy seems to have a mixed morphology, showcasing both characteristics of an elliptical galaxy and a spiral galaxy. A slight asymmetry in the galaxy's overall structure is apparent, which could potentially indicate a past or ongoing minor merger event.
