The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears largely spheroidal with a dominant bulge component, showing high degree of circularity. The color profile suggests a population of older stars, with a redder hue dominating the central regions, trending towards a more yellow color in the outer regions. There is no significant evidence of strong spiral arm structure, or active star formation. There is a possible object nearby, possibly a companion galaxy. The light from this galaxy may be from the intermediate mass range. The galaxy does not appear to be strongly disturbed, suggesting it is likely not undergoing a major merger event.
