The galaxy appears as a moderately luminous elliptical object. Its morphology suggests a relatively smooth, spheroid-dominated structure. The galaxy exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually towards the outer edges. The core of the galaxy presents a yellowish hue, potentially indicative of an older stellar population. The elongation suggests a moderate degree of flattening, classifying it somewhere between round and cigar-shaped. There is no readily apparent evidence of significant disk features or spiral arms, or major mergers. Minor disturbances cannot be ruled out, but are difficult to discern.
