The galaxy presents as a centrally concentrated, elliptical morphology, with a smooth, spheroidal structure. There is little evidence of spiral arms or a prominent disk component. The central region exhibits a bright, yellowish-white hue, suggesting a higher concentration of older stellar populations. Moving outwards from the core, the galaxy displays a gradual decrease in luminosity, transitioning to a more diffuse, reddish-orange color. This color gradient may indicate an increasing prevalence of older, redder stars in the galaxy's outer regions. There are no obvious signs of ongoing major mergers, strong tidal features, or significant dust lanes. Minor disturbances may be present, but no distinct indications. The overall appearance suggests a relatively evolved, quiescent system.
