The galaxy presents as a somewhat elongated, smooth structure. It appears to be elliptical in morphology, with a cigar-like shape. The light distribution shows a concentrated central bulge that emanates outward into a diffused envelope. The color profile displays a predominantly yellowish-orange hue which could be indicative of an older stellar population. Evidence of disturbances is seen in the faint, extended tail-like features that may suggest ongoing or past interactions or minor tidal disturbances.
