The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The light distribution appears roughly circular, with a gradual decrease in brightness moving outward from the core. There is a lack of any discernable spiral arm structures or prominent dust lanes. The color profile suggests an older stellar population, indicated by the reddish-yellow hue. This color is more pronounced towards the center of the galaxy, potentially signifying a higher concentration of evolved stars within the bulge. The galaxy shows no visual signs of ongoing major mergers or significant tidal disturbances. Overall, it appears to be a fairly relaxed and evolved system.
