The galaxy appears as a centrally concentrated object, exhibiting a smooth morphology. The light distribution suggests a dominant spheroidal component, with a high degree of central concentration. The galaxy displays a mostly featureless profile, lacking any prominent spiral arms or obvious dust lanes, suggesting a relatively homogenous stellar population. The color appears yellowish, consistent with an older stellar population. The galaxy is not perfectly spherical. There may be some slight asymmetry or a faint tidal feature, however, there is no clear evidence of ongoing major mergers or significant disturbances. Overall, this galaxy appears to be a relatively evolved system.
