The galaxy presents with a generally smooth morphology, but with some discernible features. The primary structure appears centrally concentrated and somewhat elongated. The central region displays a yellowish hue, suggestive of an older stellar population. Extending outwards, a faint, bluish halo or disk is visible. This blue color implies the presence of younger, hotter stars and ongoing star formation. A possible tidal tail or extension is seen at the end, further suggestive of potential gravitational interactions or past mergers. The overall impression is of a galaxy transitioning from a smoother elliptical to something more irregular, potentially triggered by interaction or internal dynamics.
