The galaxy presents as a spiral type, exhibiting a disk-like structure with defined spiral arms. The arms are not tightly wound, suggesting an intermediate spiral morphology. There's evidence of ongoing star formation within these arms, indicated by the presence of bluer hues that contrast with the generally yellower or redder light from older stellar populations.

A central bulge is apparent, not dominating the overall structure. The light from this bulge is notably brighter than the disk, implying a higher density of stars and older stellar populations. There may be a weak bar feature spanning across the central region.

The galaxy's overall morphology suggests that it is relatively isolated and undisturbed with an estimated mass of about 10^9 solar masses. The rate of star formation appears to be moderately low.
