The galaxy presents a generally smooth and centrally concentrated morphology. The light distribution appears relatively even, exhibiting no strong spiral arm structures or prominent dust lanes within the galaxy's disk. It appears to be an elliptical or lenticular galaxy, based on the lack of spiral arms and dominance of the bulge light. There is a slight elongation; it is neither perfectly circular nor significantly cigar-shaped. A subtle color gradient exists, with the central region appearing more yellowish. The overall color suggests a galaxy populated primarily by older stars and low star formation rates. There is no indication of recent major merger events, and the galaxy appears relatively undisturbed.
