The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. Its overall shape is elongated, appearing somewhat cigar-shaped, suggesting a deviation from a perfectly spherical form. The light distribution indicates a concentrated core region, possibly harboring an active galactic nucleus or a dense stellar population. The color gradient transitions from a yellowish-white core to a bluer, though faint, outer halo, which may indicate ongoing or recent star formation activity at a relatively low rate, along with an older stellar population dominating the core. There is no apparent evidence of strong tidal interactions, major mergers, or significant dust lanes within the visible structure of the galaxy. The outer edges of the galaxy are diffuse and difficult to define precisely against the background sky.
