The galaxy presents a largely smooth and round morphology, indicating a probable classification as an elliptical galaxy or a lenticular galaxy. The central region is bright and concentrated, gradually fading outwards. There is a subtle color gradient from the core, with bluer tones slightly more pronounced in the inner regions and a gradual shift towards redder hues in the outer regions of the galaxy, which could suggest some level of recent star formation, although the overall smooth appearance suggests that this galaxy does not have very active star formation. There is no clear indication of spiral arms or a well-defined disk structure in the image. A slight asymmetry or minor disturbance in the shape may be indicative of a possible past merger event, but there is no evidence that this galaxy is actively merging with another.
