The galaxy presents as a centrally concentrated object with a generally smooth appearance. The morphology is largely spheroidal, exhibiting a moderate ellipticity. The color gradient suggests a potentially older stellar population, with the core appearing yellowish, indicative of a greater prevalence of redder stars. There is faint indication of possible disturbance or tidal features extending from the main body of the galaxy, but the primary structure remains intact. A faint plume may extend away from the right side of the galaxy and suggests a low intensity interaction in its recent past. The galaxy exhibits a slight fuzziness, potentially due to the presence of unresolved structures or dust.
