The galaxy appears to be an elliptical or lenticular type, characterized by a smooth, diffuse light distribution. There is a concentration of light toward the center, suggesting a bulge. The overall shape is somewhat elongated but generally round, lacking a distinct spiral arm structure. No significant dust lanes or regions of active star formation are readily apparent in this image. The color profile suggests an older stellar population, with a greater contribution from redder wavelengths. Indications of minor disturbances could potentially be present.
