The galaxy presents a generally smooth, elliptical morphology, though subtle features and a possible disk structure cannot be entirely ruled out. The galaxy's light profile appears concentrated towards the center, exhibiting a bright, compact core that gradually fades into the outer regions. The shape seems to be somewhat elongated, deviating slightly from perfect circularity, tending toward an intermediate shape with a slight cigar-like appearance. There is a possible minor disturbance or interaction to the left of the galaxy, but it does not appear to be in the process of a major merger. The galaxy exhibits colors that trend towards the redder end of the spectrum, suggesting an older stellar population and relatively low star formation activity. Based on the color, the galaxy has a considerable amount of mass.
