The galaxy presents an elliptical morphology, displaying a smooth, centrally concentrated luminosity profile. The core region exhibits a yellowish-white hue, suggestive of an older stellar population dominating the light output. Progressing outwards from the core, the color transitions to a slightly redder tone, hinting at the potential presence of dust or a change in the age of the stellar population. Overall, the galaxy appears relatively undisturbed with no obvious signs of recent major merger activity or strong tidal features. The observed shape is more akin to an elliptical morphology, with a noticeable elongation that can be described as between round and cigar shaped. Although, some features or possible faint disk structures may exist. These possible features appear to be partially obscured or are embedded within the smooth light distribution. The lack of prominent blue color suggests a relatively low rate of on-going star formation. 
