The galaxy presents as a relatively smooth, elliptical-like structure. A concentrated central bulge dominates its appearance, exhibiting a bright, yellowish-white color, which likely indicates an older stellar population. The outer regions of the galaxy appear more diffuse and exhibit a fainter, slightly reddish hue, potentially resulting from dust absorption and a declining density of stars. The overall shape is closer to round than to cigar-shaped, with the smooth appearance potentially suggesting a lack of recent major mergers or significant star formation activity. Faint hints of structure may be present within the outer halo, though these are difficult to definitively identify, and the majority of the galaxy appears undisturbed.
