The galaxy presents as a relatively smooth, elliptical-like structure. Its core appears concentrated and bright, with luminosity decreasing gradually towards the outer edges. The overall color is yellowish-white, suggesting a stellar population dominated by older stars. There is a slight asymmetry in the outer regions; however, there is no clear indication of spiral arms or active star formation regions. The galaxy is approximately 2.6 kpc across. There is no visible evidence of a major merger or tidal disturbances, but minor irregularities may be present. The galaxy is estimated to have a stellar mass in the range of 10^10 solar masses, with a relatively low rate of star formation.
