The galaxy appears as a relatively compact object. Its central region exhibits a high surface brightness, suggesting a dense concentration of stars. The overall morphology appears elliptical, lacking any obvious spiral arm structures.  There is a suggestion of a slight asymmetry or disturbance in the outer regions of the galaxy, potentially indicating a minor interaction or past merger event. The object is centrally condensed, with a smooth brightness profile extending outwards, though the outer regions are faint and difficult to resolve.
