The galaxy presents as a relatively smooth, elliptical structure. Its light profile appears centrally concentrated, with a gradual decrease in luminosity towards the outer edges. The core region shows a bright concentration, likely indicating a high density of stars. There is a slight asymmetry in the outer regions of the galaxy, possibly indicative of a past or ongoing minor interaction or disturbance. The galaxy's color is primarily yellowish-white, suggesting a stellar population dominated by older, lower-mass stars. There is no clear evidence of spiral arms or significant dust lanes. A faint hint of blue tinge in the outer regions may be present, potentially indicating the presence of some younger stars, but the overall impression is of an evolved system. There is a potential companion galaxy in close proximity which could have caused the disturbance mentioned above.
