The galaxy presents as an elliptical or lenticular morphology, displaying a generally smooth light distribution. The central region exhibits a bright, concentrated core, indicative of a spheroidal component. The overall color is skewed toward the redder end of the spectrum. The galaxy's shape appears somewhat elongated. A faint, distorted structure is potentially observable within the outer regions. There appears to be minimal evidence of active star formation. Possible gravitational interaction seems to exist with a smaller object on the lower left side.
