The galaxy presents as a luminous, elliptical-like structure. The central bulge appears bright, with a yellowish-white hue, suggesting a population of older stars. The overall shape is somewhat flattened, with a clear major axis. Extending outward from the bright central region, the light gradually fades, indicating a relatively smooth stellar distribution. Faint blueish tendrils can be seen on the edge of the disk, which may indicate active star formation. No distinct spiral arm structure or prominent dust lanes are readily apparent. There is no sign of interactions with any other galaxies. Overall the galaxy appears to be of moderate size and mass.