The galaxy presents as a luminous, diffuse object with an overall elliptical morphology. Its central region exhibits a higher surface brightness, suggesting a concentration of older stars. Moving outward from the core, the light gradually fades into a broader, less defined halo. There are slight variations in the halo, indicating areas with potential disturbances or ongoing star formation, although a lack of distinct spiral arms or strong features suggests these are not pronounced. The galaxy is elongated, appearing more in between a round and cigar-shaped structure. Some indicators point to minor disturbances, yet an absence of clear tidal tails suggests these interactions are not major merging events. The overall color profile suggests a mix of stellar populations, with possibly more evolved stars dominating the central bulge and potentially younger stars contributing to the halo's color.
