The galaxy appears as a moderately luminous, elliptical structure. Its morphology suggests a relatively smooth distribution of light, concentrated towards the center and gradually decreasing outwards. There are no prominent spiral arms or distinct features indicating active star formation regions like HII regions. The core exhibits a yellowish hue, possibly indicating an older stellar population. The galaxy shows an intermediate ellipticity, appearing as an oval shape, more elongated than circular, but not exceedingly cigar-shaped. There is a very slight asymmetry in the outer regions, but no clear signs of a major ongoing merger. A small disturbance may be present. The overall light profile suggests a galaxy with a fairly high mass, and very little star formation activity.
