The galaxy presents a generally smooth morphology, with a concentrated central bulge that appears to be a yellow-gold color. This suggests an older stellar population within the bulge. Extending outwards from this central region is a less defined, fainter disk. The disk seems to be at an angle with respect to the line of sight. There may be a faint hint of spiral structure but there is no resolution to confirm this. The overall shape could be described as somewhere between round and cigar-shaped. There is a possible sign of a minor disturbance to the galaxy, as shown by a possible tidal tail. From these observations, it is likely the galaxy is a disk galaxy.
