The galaxy presents a generally smooth, elliptical morphology. The light profile exhibits a radial gradient, with a bright, concentrated core that gradually fades into a more diffuse halo. There is no discernible spiral arm structure or prominent dust lanes visible in the image. The color appears to be dominated by redder wavelengths, with a subtle shift towards bluer tones in the outer regions. This suggests the presence of an older stellar population, with possible recent star formation in the outskirts. The galaxy displays an approximate diameter of 5 Kpc. No obvious signs of tidal disturbances or ongoing mergers are apparent, indicating a relatively undisturbed, quiescent system. Overall, this galaxy appears to be a mature, early-type galaxy with a substantial mass and very little star formation.
