The galaxy presents as a somewhat elliptical form, with a relatively smooth light distribution. The core region appears luminous and concentrated, exhibiting a yellowish hue, possibly indicative of an older stellar population. This central bulge is surrounded by a more diffuse and extended halo that transitions to a slightly bluer color, which may suggest the presence of younger stars or ongoing star formation in the outer regions. The overall structure lacks prominent spiral arms or significant dust lanes, indicating that it's not a classical spiral galaxy and may classify as an elliptical or lenticular galaxy. There are hints of minor disturbances or asymmetries, but the overall appearance is mostly undisturbed.
