The galaxy appears as a moderately sized, relatively smooth object. It exhibits a generally elliptical morphology, displaying a shape that is neither perfectly spherical nor highly elongated. The light distribution within the galaxy seems to be centrally concentrated. The color profile suggests a population of older stars, with a tendency toward redder hues. There is no obvious spiral arm structure or strong dust lane features visible in the image. The overall structure appears undisturbed, showing no clear evidence of ongoing major mergers or significant tidal interactions. Faint, diffuse extensions might exist, but they are not pronounced.