The galaxy presents a generally smooth, elliptical morphology with minimal discernible disk features. It exhibits a concentrated central bulge that dominates the overall luminosity. The color profile suggests a population of older stars, indicated by the yellowish-red hues in the central region and the galaxy's halo. No distinct spiral arms or prominent dust lanes are observed. There is a faint bluish tinge along the edges, perhaps indicating limited star formation activity in those regions. The galaxy appears relatively isolated, showing no strong signs of tidal interactions or ongoing mergers with other galaxies, though some distortion in the outer halo cannot be ruled out. Overall, the galaxy exhibits characteristics consistent with a mature elliptical galaxy, potentially transitioning from a phase of active star formation to quiescence.
