The galaxy presents as an elongated, elliptical shape with a relatively smooth texture. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish hue indicative of an older stellar population. The outer regions appear fainter and display a more diffuse, reddish tint, possibly resulting from a mix of older stars and dust. There is little indication of distinct spiral arms or active star formation regions, and the galaxy appears relatively undisturbed, lacking significant tidal features or signs of a major merger. The galaxy's structure is mostly smooth, with a gradual change in brightness from the center to the outer edges, with a moderate redshift suggesting a relatively distant location. The overall appearance suggests a passively evolving galaxy with a significant fraction of its stars in older populations.
