This galaxy presents as a relatively compact, centrally concentrated object. The light distribution appears smooth, lacking any prominent spiral arm structures or a clearly defined disk. It seems to be a fairly spheroidal galaxy. There is an absence of any obvious dust lanes or features indicative of ongoing major mergers or tidal disturbances. The galaxy exhibits a color gradient, with the core appearing more reddish/pinkish, possibly suggesting an older stellar population and/or significant dust obscuration in the central region. The outer regions of the galaxy appear to be bluer in comparison, indicating younger stars. Based on the smooth light profile and color properties, this galaxy might be an elliptical or lenticular galaxy.
