The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color profile suggests an older stellar population, with a dominant yellowish hue indicative of evolved stars. There is little evidence of spiral arm structures or significant dust lanes, indicating a lack of ongoing major star formation. The galaxy appears largely undisturbed, exhibiting no obvious signs of a recent major merger or tidal interactions. The galaxy has a moderately compact size and a nearly round shape. The overall characteristics point towards a passively evolving galaxy, potentially a lenticular or elliptical type.
