This galaxy exhibits a complex morphology, displaying characteristics of both a smooth elliptical component and a more disturbed, disk-like feature. The central region is dominated by a bright, concentrated spheroid, possibly indicative of an older stellar population with a relatively smooth light distribution. There is evidence of a ring like feature in this central region. A fainter, extended structure extends from one side of the core, exhibiting irregular shapes and a lower surface brightness, it appears to be a tidal tail. Its color suggests ongoing star formation activity, though it's difficult to ascertain the full extent of this activity given the resolution. The overall structure suggests either an interaction with another galaxy or an internal dynamic process that has significantly perturbed its morphology. Further spectral analysis would be needed to clarify the nature of the observed disturbances and better constrain the galaxy's evolutionary history.
