The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that is slightly elongated in shape. The core region appears to be the brightest and is characterized by a yellowish-white hue, possibly indicative of an older stellar population. Moving outward from the core, a more diffuse and less luminous halo is observed. This halo is characterized by a blueish hue. Overall, the light distribution is relatively even, suggesting a lack of significant spiral arm structure or irregular features. The shape is elongated, appearing cigar-shaped. There is no obvious evidence of a major merger, or strong tidal disturbances in the immediate vicinity of the galaxy.
