The galaxy presents an elliptical morphology. The light distribution appears smooth and concentrated towards the center, suggesting a relatively old stellar population. A slight elongation is visible in the galaxy's shape. Color gradients indicate a yellowish central bulge, possibly indicative of older, redder stars concentrated towards the core. Fainter, bluer hues in the outer regions might suggest the presence of younger, star-forming populations. No strong dust lanes or prominent spiral arm structures are discernible. There are no obvious signs of tidal interactions or major mergers. The galaxy appears to be relatively isolated and undisturbed.
