The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be a disk galaxy that is viewed at an angle. The central bulge exhibits a brighter, more concentrated luminosity, characterized by a yellowish-white hue, potentially indicating a population of older stars. The outer regions of the galaxy display a fainter, bluer tint, suggestive of ongoing, albeit subtle, star formation. There are some irregularities present, suggesting minor tidal disturbance in the past or ongoing minor accretion events, but the overall structure is largely undisturbed.
