The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. The overall shape suggests a moderate degree of ellipticity, appearing somewhere between round and cigar-shaped. There is no obvious evidence of spiral arms or a well-defined disk structure. The galaxy's color is predominantly yellowish-white, indicating a likely older stellar population. There is no clear indication of ongoing major merging events, although a minor disturbance cannot be completely ruled out. The galaxy displays a lack of prominent dust lanes or active star-forming regions, suggesting a relatively quiescent state.
