The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a concentrated luminosity with a yellowish-white hue, suggesting an older stellar population. The outer regions display a fainter, bluer tinge, indicative of possible recent star formation activity, although it is relatively subdued. There is no obvious spiral arm structure, and the galaxy appears relatively smooth and undisturbed. The galaxy shows a possible presence of a disk and the light distribution suggests that it might be an edge-on spiral galaxy or an elliptical galaxy. There are no signs of any major mergers or tidal disturbances.
