The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. The light profile suggests a relatively old stellar population, with a yellow-red hue dominating the central region. There is little evidence of spiral arms or significant dust lanes. The galaxy's shape is generally elliptical, and the outer regions of the galaxy seem to fade gradually into the background sky, indicating a lack of sharp edges or truncation. No signs of any recent major merger activity or tidal disturbances are visible.
