The galaxy presents as a luminous, elliptical structure, approximately 8 kpc in radius. It exhibits a smooth, featureless morphology, lacking prominent spiral arms or significant dust lanes. The central region shows a bright, concentrated core which may be evidence of an active galactic nucleus or a dense stellar population. The color profile suggests an older stellar population, characterized by a dominant yellowish hue. There may be a faint, diffuse halo surrounding the main body of the galaxy, subtly extending the observed diameter. Evidence of significant merger activity is absent, with only minor disturbances potentially indicated by slight irregularities in the outer regions of the galaxy. Overall, the galaxy appears to be a relatively massive, quiescent system with a low star formation rate.
