The galaxy presents as a relatively smooth, elliptical structure with a dominant central bulge. The light profile appears centrally concentrated, exhibiting a gradual decline in intensity moving outwards from the core.  The galaxy exhibits a yellowish-red hue, possibly indicative of an older stellar population, implying reduced star formation.  There is little evidence of spiral arms, dust lanes, or other distinct features typically associated with younger, disk-dominated galaxies. The overall morphology suggests a system that is relatively undisturbed, without signs of major mergers or tidal interactions. The galaxy appears approximately round.
