The galaxy presents as an elliptical morphology, appearing largely smooth and featureless in this image. The color gradient suggests a central bulge that is yellower in hue, indicating an older stellar population and a potential lack of ongoing star formation in the core. The outer regions exhibit a bluer tint, possibly indicative of a younger stellar population or residual star formation activity at the periphery. The galaxy exhibits a moderately elongated shape, falling somewhere between a perfectly round and a cigar-like form. No signs of major mergers or significant tidal disturbances are evident. Faint disk-like characteristics are hard to determine but might be present.
