The galaxy presents a roughly circular morphology with a prominent central bulge. The bulge exhibits a concentrated luminosity, suggesting a high density of stellar population. Moving outward from the core, the galaxy transitions into a less defined disk structure. This disk shows faint spiral arms that are tightly wound. Indications of ongoing star formation are present within these arms, marked by a subtle bluish hue.

Overall, the galaxy's light distribution appears relatively smooth, with no dramatic features or asymmetries immediately apparent. There are indications of a possible minor interaction with another galaxy in the form of a faint tidal stream.
