The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical, with the isophotes gradually fading outwards from the core. There is a pronounced central bulge, displaying a bright, compact region. Moving outward from the core, the luminosity decreases steadily. The galaxy does not exhibit any prominent spiral arm structure or significant dust lanes in the image. The color profile reveals a slight reddening towards the central regions, while the outer regions may have a subtle bluer hue. There is no evidence of strong tidal features, such as extended streams or shells, suggesting it is not undergoing any major merger events. The galaxy appears relatively isolated, with no obvious nearby companion galaxies visibly interacting.
