The galaxy presents as a relatively smooth, concentrated object, appearing largely elliptical in form. A bright central bulge dominates its structure, exhibiting a yellowish hue, indicative of an older stellar population. Moving outward from the core, the luminosity decreases gradually, with hints of a slightly bluer disk component surrounding the central bulge. The outer edges are somewhat diffuse and indistinct, lacking sharp boundaries. There may be some minor disturbances or irregularities present in the overall structure suggesting interaction with another galaxy. The galaxy shows little evidence of prominent spiral arms or dust lanes.
