This galaxy appears to be a relatively smooth and rounded system, likely an elliptical or S0 type. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity outwards. There may be a subtle disk component but it is very faint. There is no strong evidence of spiral arms or significant dust lanes. The galaxy exhibits a yellow-red color, which implies an older stellar population and a lack of significant ongoing star formation. Any features that suggest mergers are weak or nonexistent, suggesting a relatively undisturbed evolutionary history for this galaxy.
