The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange in color, indicative of an older stellar population. The outer regions of the galaxy display a bluer hue. The galaxy shows no distinct spiral arm structure. There are no apparent signs of any ongoing major merging activity, although a minor disturbance is not fully ruled out. The overall shape appears elongated, closely resembling a cigar shape. The inferred stellar mass is moderate, with relatively low levels of star formation.
