The galaxy presents as a centrally concentrated object, roughly elliptical in shape. It exhibits a smooth, yellowish-orange color profile, suggesting an older stellar population and a lack of significant ongoing star formation. There is no visible evidence of spiral arm structure or a prominent disk. The galaxy appears relatively isolated, with no clear signs of major tidal interactions or ongoing mergers, though subtle irregularities in its outer isophotes could indicate minor past interactions. The galaxy appears moderately massive.
