The galaxy presents an elliptical morphology, displaying a smooth, concentrated light profile that suggests an older stellar population. A prominent, bright central bulge dominates the structure, indicative of a substantial concentration of stars. Moving outward from the core, the light gradually fades, showing a diffuse halo surrounding the main body. A slight asymmetry or minor disturbance can be observed to one side, with a faint reddish tendril. This could be the result of a past or ongoing interaction with another galaxy, though no obvious companion is seen. The overall color suggests a mix of stellar ages, with a predominance of older, redder stars in the bulge and possibly a slightly younger, bluer population in the outer regions.
