The galaxy presents as a relatively compact object with an elliptical morphology. It is composed of a bright, concentrated central bulge that dominates the galaxy's overall luminosity. The color profile suggests a redder stellar population, particularly concentrated towards the core. Fainter, bluer regions are observed extending asymmetrically away from the bulge, implying ongoing or recent star formation, potentially in a disk-like structure. There is some distortion visible, suggesting a possible interaction. Overall, the galaxy appears to be in a transitional state, possibly evolving from a more active spiral to a quiescent elliptical.
