The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light profile appears largely featureless, suggesting an older stellar population. There is minimal indication of spiral arms or significant dust lanes. The galaxy's core region exhibits a yellowish hue, transitioning to a redder tone towards the outer regions, which could suggest a gradient in the age of the stellar population. The galaxy appears relatively isolated. No obvious signs of ongoing major mergers or tidal disturbances are apparent, although subtle disturbances or minor interactions cannot be ruled out without higher resolution data.