The galaxy presents as a relatively compact and luminous entity. Its morphology appears largely smooth and elliptical in shape, lacking prominent spiral arms or a well-defined disk structure. The light distribution is concentrated towards the center, suggesting a significant central bulge. There is some indication of minor disturbances or irregularities in the galaxy's structure. The color indices imply that the stellar population is dominated by older, redder stars. The galaxy exhibits a moderate amount of star formation, but it is not exceptionally active. Based on the mass estimates, it is a moderately massive galaxy.
