The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. Its light profile suggests an elliptical morphology, with the central region appearing brightest and gradually fading outwards. There is little indication of spiral arms or significant disk-like structure. The galaxy appears to have a reddish hue overall, suggestive of an older stellar population, or significant dust obscuration, with minimal evidence of recent, ongoing star formation. There is no obvious signs of major disturbances or merging events. A subtle tidal feature may be present on one side.
