The galaxy presents a generally smooth and rounded morphology. Its light profile suggests a dominant spheroid component, with a likely elliptical classification. The central region appears more concentrated, fading towards the outer edges. Some degree of tidal disturbance, possibly indicative of past or ongoing interactions, appears to be present, particularly in the form of a diffuse outer halo or shell-like structure. This would suggest the possibility of minor mergers. The color distribution is relatively uniform, but there might be a slight shift in the reddish or yellow end of the spectrum. Overall, the observed features indicate a galaxy of considerable mass.
