The galaxy presents as a relatively small, elongated object. Its morphology suggests a possible elliptical or lenticular classification due to its smooth, featureless appearance. The color profile appears to be predominantly redder, indicating an older stellar population. The light is concentrated towards the center, with a gradual fading towards the edges, a characteristic of spheroidal systems. No spiral arms or significant dust lanes are discernible in this image. The general form factor appears cigar-shaped. There is no obvious sign of recent or ongoing merging activity.
