The galaxy appears to be a relatively smooth and rounded elliptical type, exhibiting a concentrated central bulge. There is little evidence of significant spiral arm structure or prominent dust lanes. The light is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. Color gradients appear to be minimal, with a generally yellowish hue, suggesting an older stellar population and low rate of ongoing star formation. The galaxy appears relatively isolated, without obvious signs of interaction or ongoing mergers, although some minor disturbances cannot be ruled out. The overall morphology suggests a galaxy that is in a relatively evolved state.
