The galaxy presents a primarily smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decline in surface brightness outwards. The dominant color is a yellowish-orange hue in the core region, suggesting an older stellar population. Fainter, bluer extensions are observed, indicating the presence of some star formation, albeit at a low rate. The galaxy appears somewhat elongated, with an axial ratio that suggests a deviation from a perfectly spherical shape. There is some evidence of a minor disturbance in the galactic structure, although the galaxy is not in the throes of a major merger. The presence of faint tidal features or disrupted structures is not prominent, yet it's possible there's a small interaction going on.
