The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a morphology that leans towards being elliptical in shape, though not perfectly spherical. There is a slight elongation but it is not a highly flattened disk system. There is no obvious, grand design spiral structure.

The light profile seems to be dominated by older stellar populations, with a generally redder color, with hints of some bluer light, indicating the presence of younger stars or regions of ongoing star formation. There is no strong evidence of a major ongoing merger, although the possibility of minor disturbances or past interactions cannot be entirely ruled out based on the image alone. The galaxy does not appear to be particularly active in terms of star formation.
