The galaxy presents as a somewhat elliptical object with a smooth, concentrated central bulge. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population.  Surrounding the central bulge, a fainter, less defined disk is observed. The disk appears to be only subtly discernible and also exhibits a yellowish-orange hue, with a slight hint of a bluer component, possibly indicative of more recent, though subdued, star formation.  No prominent spiral arms are apparent. The overall morphology suggests a galaxy transitioning between classifications, potentially a late-type spiral or early-type elliptical. There are subtle asymmetries within the disk structure, hinting at a potential past interaction or minor disturbance event, though no strong evidence of a major ongoing merger is immediately visible. The galaxy appears relatively isolated.
