The galaxy presents as a flattened, elliptical structure with a major axis significantly longer than its minor axis, appearing somewhat cigar-shaped. The color profile is generally smooth, exhibiting a yellowish hue, indicative of an older stellar population. There is no discernible dust lane or spiral arm structure. The overall light distribution suggests a relatively smooth stellar density gradient, with a brighter core fading gradually towards the edges. There is no apparent evidence of recent or ongoing major mergers or tidal disturbances. The galaxy appears relatively undisturbed.
