The galaxy presents as a relatively symmetrical, disk-shaped structure with a concentrated central bulge. A subtle, slightly distorted spiral arm structure is tentatively observable. The disk itself appears relatively smooth in texture, with a distribution of light that suggests ongoing star formation. The galaxy exhibits a slightly elongated morphology but is predominantly round. No major signs of recent or ongoing merging events are readily apparent, though minor disturbances are subtly discernible in the disk. The color distribution is indicative of a significant stellar population, including both older, redder stars and younger, bluer stars.
