The galaxy presents a primarily elliptical morphology, appearing largely smooth in structure with a dominant central bulge. There is a slight elongation to the galaxy's shape, deviating marginally from a perfectly circular profile, perhaps tending towards a cigar shape. The color profile is characterized by a reddish-orange hue, suggesting a population of older stars with lower rates of ongoing star formation.  There are suggestions of minor disturbances in its morphology, the galaxy could be undergoing some sort of gravitational interaction. The galaxy has no spiral arm structures and the image data indicates a relatively high mass.
