The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outwards, lacking distinct spiral arm structures or prominent features such as dust lanes. The galaxy appears largely spheroidal with a high degree of central concentration. The color profile suggests a stellar population dominated by older, redder stars, likely indicating a relatively low current star formation rate. There is no noticeable tidal disruption or morphological asymmetry to suggest a recent major merger event, although minor disturbances may be present but are not obvious. Overall, this appears to be a relatively undisturbed, evolved elliptical galaxy.
