The galaxy presents as a singular, relatively smooth, and concentrated structure. It exhibits an elliptical morphology, appearing somewhat elongated, but not excessively so. The color profile suggests a dominant population of older stars, indicated by the yellowish-red hue, consistent with minimal ongoing star formation. There may be some minor disturbances within the galaxy itself but shows no apparent signs of major mergers or tidal interactions with other galaxies. The shape is not perfectly round, trending towards an intermediate spheroidal form. There is no evidence of a spiral structure, disk component or distinct nucleus visible at this resolution.
