The galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The primary color is a yellowish-orange hue, suggesting a population of older stars. The light profile seems to fade gradually from the core outwards. There is subtle evidence of a disk-like component, but it's faint and largely obscured by the dominant spheroid. There is a slight asymmetry in the light distribution, with some disturbance in the galaxy structure on one side, but without strong signs of an ongoing major merger. The galaxy is elongated, trending toward a cigar shape. Star formation appears to be relatively low. Overall, the galaxy presents as a mature system.
