The galaxy presents as a moderately bright, disk-like structure with a relatively smooth appearance. It is observed to have a slightly elongated shape, appearing more 'in-between' round and cigar-shaped. The central bulge is not particularly prominent. There are faint signs of spiral structure, but they are not well-defined. The galaxy exhibits a relatively uniform color distribution, with a slight concentration of bluer light towards the outer regions of the disk. There's no significant evidence of tidal tails or major disturbances, suggesting it is not currently undergoing a major merger. Close inspection indicates this galaxy is experiencing a low rate of star formation.
