The galaxy appears as a relatively bright, centrally concentrated object. It exhibits a smooth, rounded morphology, lacking prominent spiral arms or a well-defined disk structure. The light distribution suggests an elliptical or lenticular classification. There is a subtle color gradient, transitioning from slightly bluer hues in the outer regions to redder tones towards the core, possibly indicative of older stellar populations dominating the central region. There's no evidence of significant ongoing mergers or major tidal disturbances. A faint, extended halo is suspected, contributing to the galaxy's overall luminosity. There are no dust lanes or obvious signs of active star formation.
