The galaxy presents a primarily smooth morphology, with a high degree of central concentration. Its overall shape appears to be elliptical, deviating slightly from a perfect circle, leaning more towards a moderate elongation. There is no obvious dust lane or spiral arm structure visible. The color profile suggests an older stellar population, with a yellowish hue dominating the central bulge. Fainter, reddish extensions are possibly indicative of evolved stars. The galaxy appears to be relatively isolated, exhibiting no signs of major tidal disturbances or interaction with other nearby galaxies. Any minor disturbances are difficult to determine at this resolution.
