The galaxy exhibits a generally elliptical morphology, appearing largely smooth and relatively undisturbed. There is little evidence of distinct spiral arms or a prominent disk structure. The central region appears to be more concentrated and slightly yellowish. A faint, extended halo is visible, surrounding the brighter central region. The color profile suggests a population of older stars with a low star formation rate. The galaxy seems to be relatively isolated, showing no significant signs of tidal interactions or ongoing mergers with other galaxies. There may be a very slight asymmetry.
