This galaxy presents as an elliptical type, exhibiting a smooth, concentrated structure with a prominent central bulge. The galaxy displays an overall yellowish-red hue, suggesting an older stellar population and potentially a lower rate of current star formation. The luminosity appears centrally concentrated, gradually decreasing outwards from the core. There is a slight flattening of the galaxy disk, hinting at a possible disk component but without any resolved spiral arms. The outer edges appear diffuse, with no sharp cut-off in luminosity. There is minimal, if any, observable dust or gas lanes. It appears to be a fairly isolated galaxy, without any obvious signs of tidal disruption or ongoing interactions with other galaxies.
