The galaxy presents an elliptical morphology, elongated along a major axis. A smooth light distribution characterizes the galaxy, suggesting an older stellar population. The core region exhibits a concentration of light, appearing yellow-orange in color, possibly indicative of older, redder stars dominating the nuclear region. Fainter bluish hues are observed on the outer edges of the galaxy. No distinct spiral arms or significant dust lanes are readily apparent. The outer regions gradually fade into the background sky, displaying a diffuse halo structure. There are no obvious signs of recent or ongoing major mergers, though subtle disturbances cannot be entirely ruled out at this resolution.
