The galaxy presents a largely smooth and elliptical morphology. It appears as a concentrated spheroid of light, with a relatively high degree of central concentration. The color profile indicates a dominant population of older stars, given the redder hue evident around the brighter center. There is little evidence of spiral arm structure or significant dust lanes. The overall shape is approximately round. There are no obvious signs of ongoing merger activity or major tidal disturbances, suggesting it is a relatively isolated system or has reached a late stage in a merger process where tidal features have dissipated. The galaxy is of an intermediate luminosity and mass.
