The galaxy presents as a luminous, yellowish-orange elliptical. Its morphology appears relatively smooth, lacking distinct spiral arm structures or prominent dust lanes. The light distribution suggests a centrally concentrated brightness profile, with luminosity decreasing gradually towards the outer edges. There is a slight elongation in the galaxy's shape, deviating somewhat from a perfect circular form; the shape might be described as being in-between round and slightly cigar-shaped. There is no strong evidence of ongoing or recent major mergers. The absence of clearly defined star-forming regions within the galaxy suggests a relatively low star formation rate, consistent with a population dominated by older stars. Faint hints of blue are found on the edges of the galaxy.
