The galaxy presents a generally smooth, elliptical morphology. It exhibits a central bulge that appears relatively bright and concentrated. A disk structure is suggested by the slightly elongated shape, although it lacks the distinct spiral arms typically associated with grand design spirals. The galaxy's color profile indicates a population of intermediate-age stars. The absence of prominent dust lanes and star-forming regions suggests a relatively low star formation rate. There may be some tidal disturbances present, indicating that there may have been a minor merger or interaction in its recent past. 
