The galaxy presents a mostly smooth, elliptical morphology. It exhibits a concentrated central bulge, with light intensity decreasing gradually outwards. There is very little evidence of spiral arm structure or prominent dust lanes. The overall color appears to be a yellowish-red hue, suggesting a population of older stars and a relatively low rate of ongoing star formation. The galaxy has a relatively circular appearance, showing only very minor deviations from perfect radial symmetry. No clear signs of interaction with other galaxies or significant morphological disturbances are observed.
