The galaxy appears to be a relatively smooth, elliptical or lenticular type, with a concentrated central bulge. The light distribution suggests a primarily older stellar population, exhibiting a yellowish-orange hue towards the core, indicating a diminished rate of recent star formation. There's a slight asymmetry in the outer regions, with a faint, diffuse extension visible. This may be indicative of a minor tidal interaction or past merger event. The galaxy has an approximate diameter of 8.7 kpc. Overall, the galaxy presents as a well-defined, moderately massive system.
