The galaxy presents as a relatively compact object, appearing roughly elliptical in shape but exhibiting subtle irregularities. There is a dominant, bright core region that appears smooth and moderately concentrated. The light distribution falls off gradually from the core towards the outer regions. A slight elongation is noticeable along one axis, giving it a somewhat cigar-shaped appearance. The galaxy's color suggests a mixed stellar population, with a slight tendency toward bluer hues indicative of some recent or ongoing star formation activity, concentrated towards the centre. No clear spiral arm structure or prominent dust lanes are visible. There is a suggestion of faint extended emission surrounding the main body of the galaxy, possibly indicating a diffuse halo. No evidence of a major merger event or tidal disturbances is immediately apparent. The overall impression is that of a galaxy undergoing a transition from a more irregular form towards a smoother, more elliptical morphology.