The galaxy presents as a relatively compact, elliptical morphology. A bright, concentrated central bulge dominates the structure. A diffuse halo surrounds the central region, gradually fading into the background. There appears to be some asymmetric disturbance, with a faint indication of a tidal tail or potential minor merger on the right side of the galaxy. The color profile suggests the presence of older stellar populations, with a bluish hue concentrated in the central region and a gradual shift towards redder tones in the outer regions. The overall shape is somewhat elongated, but not strongly so. The smoothness of the light distribution suggests that it is likely an early-type galaxy with little ongoing star formation activity outside of its bulge.
