The galaxy presents a largely elliptical morphology, exhibiting a high degree of smoothness across its visible structure. A bright, concentrated central bulge dominates the galaxy's core, appearing to be a yellowish hue, possibly indicating an older stellar population within this region. The outer regions of the galaxy display a gradual decline in luminosity, with a bluer tint, suggesting some degree of ongoing or recent star formation activity, though at a relatively low rate. There is no obvious disk structure or prominent spiral arm features discernible in the image. Slight asymmetry might be present, though not indicative of major disturbances or ongoing merger events. Overall, the galaxy appears to be a relatively isolated system in a late stage of its evolution.
