The galaxy appears to be an elliptical galaxy with a generally smooth morphology. It is characterized by a centrally concentrated bulge. The light profile indicates it is neither perfectly round nor highly elongated but falls somewhere in between, with a slight cigar shape to the galaxy overall. There is little evidence of significant ongoing star formation activity, consistent with an older stellar population. Any disturbances appear to be minor, with no strong indication of recent major mergers or interactions. The central region has a yellowish hue, likely indicative of older stars.
