The galaxy presents a primarily smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing as a bright, unresolved core indicative of a possible bulge. The overall shape is tending toward round.

A subtle disk-like feature is suspected but not obvious, contributing to the light profile outside the core. There is a possible hint of tidal disturbance, but it would need more observations to determine if this is actually the case. The color gradient appears relatively uniform across the galaxy, suggesting an older stellar population and a low active star formation rate.
