The galaxy appears to be a relatively smooth, centrally concentrated object with a generally elliptical morphology. It exhibits a diffuse, even light distribution, suggesting a lack of prominent spiral arms or a well-defined disk structure. The core region is brighter than the surrounding areas, indicative of a concentrated stellar population. The overall color profile suggests a population of older stars, with a subtle reddening towards the center. There is no obvious evidence of ongoing major merging activity or significant tidal distortions, though there may be some minor disturbances or faint features within the galaxy's outer regions, hinting at past interactions. It seems relatively isolated and the galaxy does not appear to be actively forming many new stars. The estimated size is a few kiloparsecs in radius.
