The galaxy presents a generally smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge with a radial decrease in surface brightness outwards. The color profile suggests a predominantly older stellar population, trending towards redder hues. The galaxy's shape is elongated, appearing somewhere between round and cigar shaped, indicating a possible classification as an elliptical galaxy viewed from an angle. There are no prominent spiral arms or dust lanes discernible. Furthermore, there is no visible evidence of ongoing major merger activity or significant tidal disturbances in the immediate vicinity.
