The galaxy presents a generally smooth and rounded morphology. It exhibits a concentrated central region, likely a bulge, with a gradual decrease in surface brightness outwards. There is some evidence of a possible disk-like structure, although not clearly defined. The overall color appears relatively uniform, with a slight bluer hue, indicating some level of ongoing star formation, albeit at a moderate rate. No significant tidal features or strong signs of interaction with other galaxies are apparent, although there are some minor indications of disturbance, with possibly a very faint spiral arm structure beginning to show. Based on its apparent size and faintness, this object is estimated to be at a considerable distance.
