The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely spheroidal in shape, with only a slight deviation toward a more elongated form. The color profile suggests a population of older stars, indicated by the redder hues concentrated in the central bulge region. There's little evidence of distinct spiral arm structures or significant dust lanes, further supporting the interpretation of an evolved stellar population. The lack of pronounced blue colors suggests minimal ongoing star formation. The galaxy does not appear to be undergoing any major merging events or strong tidal interactions. Overall, the galaxy appears to be a fairly evolved elliptical galaxy with a relaxed morphology.
