The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. There is no apparent spiral arm structure or distinct features indicative of ongoing major mergers or significant tidal disturbances. The overall color profile suggests an older stellar population, evidenced by the yellowish hue. Faint hints of bluer regions may be present, possibly signifying pockets of more recent star formation, although these are not prominently displayed. The galaxy appears moderately luminous.
