This galaxy presents an elliptical morphology, with a predominantly smooth structure and a high degree of central concentration. It exhibits a relatively elongated shape, appearing more cigar-shaped than circular. The galaxy does not appear to be undergoing a major merger event, however, there is evidence of minor gravitational disturbance in the form of tidal tails which extend slightly from the central body of the galaxy. The central region has a higher concentration of older stars compared to the galaxy's peripheral areas. The blueish color suggests some ongoing star formation activity. The overall luminosity is significant, which is expected for a galaxy of this mass.
