The galaxy presents as a yellowish, elliptical structure with a centrally concentrated light profile. There is a lack of distinct spiral arms or prominent features within the visible structure. The shape appears to be generally ellipsoidal, tending toward a circular morphology, with very little elongation observed. There is no apparent indication of major mergers or significant tidal disturbances impacting the galaxy. The overall smooth appearance suggests a relatively quiescent system, potentially dominated by an older stellar population with minimal ongoing star formation activity. There is a hint of a slightly bluer hue in the outer edges of the galaxy, suggesting the presence of a younger stellar population there, although the majority of the light is redder in color.
