The galaxy appears to be a lenticular or elliptical type, exhibiting a smooth, largely featureless morphology. Its overall shape is elongated, resembling a cigar shape. The light distribution indicates a concentration of older stellar populations, with a reddish-yellow hue dominating the central regions. The galaxy shows no obvious signs of spiral arms or significant star formation, suggesting a relatively quiescent evolutionary state. There are no visually apparent disturbances indicative of recent major mergers, although minor tidal features cannot be ruled out at this resolution. The smooth light profile suggests a system dominated by an older stellar population and minimal dust obscuration.
