The galaxy appears to be a relatively smooth, elliptical type, exhibiting a mostly featureless morphology. It displays a concentrated central bulge, luminous with a yellowish hue suggesting a population of older stars. The galaxy has a roughly spheroidal shape, leaning towards an in-between rounded appearance rather than a perfect circle or elongated form. There is a faint, diffuse halo surrounding the brighter core, indicating the presence of a stellar envelope. No prominent spiral arms or significant dust lanes are discernible. The overall color suggests an evolved stellar population, potentially indicative of a relatively quiescent star formation rate. There appears to be a very minor disturbance in its form, likely due to a minor merger.
