The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge that emits strongly in the observed bands. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears to be relatively isolated with a small neighbor, and shows no obvious signs of ongoing major mergers or tidal disturbances. Its overall color is consistent with a population of older stars, suggesting a relatively low current star formation rate. The round shape dominates, with little cigar shape qualities. There is minimal presence of features or disks, and the artifact fraction is low.
