The galaxy presents a mostly smooth, elliptical morphology with an overall yellowish hue. The central region displays a slightly brighter concentration of light, suggesting a bulge. The galaxy's light is fairly uniform, with no apparent spiral arm structures or dust lanes visible in this image. The overall shape is somewhat elongated, appearing more "in between" round and cigar-shaped. There is no evidence of significant tidal disturbances or ongoing major mergers, although a subtle asymmetry might indicate a minor gravitational interaction or past merger event. Based on the color and smooth appearance, this galaxy likely has a substantial population of older stars and a low rate of ongoing star formation.
