The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology seems to be elliptical or lenticular, with a predominantly spheroidal component and no apparent spiral arms or significant disk structure. The light profile indicates a strong central bulge, and the galaxy exhibits a yellow-red color, suggesting an older stellar population with relatively little ongoing star formation, or potentially dust obscuration. There appears to be a slight elongation in its shape, but overall it is fairly round. There is no obvious indication of any major mergers or significant tidal disturbances in the immediate vicinity.
