The galaxy presents as a single, largely homogenous object, appearing nearly circular in projection. The light profile is relatively smooth, showing a strong central concentration that fades gradually towards the periphery. A distinct lack of resolved substructure such as spiral arms or prominent dust lanes is observed. The color is notably yellow-orange, suggesting an older stellar population dominating the light output. There is no obvious evidence of ongoing major mergers or tidal disturbances affecting the galaxy's morphology.
