The galaxy presents as a cigar-shaped, elongated structure. The light distribution suggests a smooth, relatively featureless morphology. A concentrated central bulge is apparent, displaying a yellowish hue. Extending outwards from the bulge, a subtle disk is implied, with a gradual decrease in luminosity towards the edges. The overall color profile indicates a population dominated by older stars, with a likely low rate of ongoing star formation. There is no obvious evidence of significant dust lanes or spiral arm structures. There is a very slight blueish tinge on the outer edges of the galaxy. The galaxy appears relatively isolated, without any obvious signs of interaction with other galaxies or tidal disturbances.
