The galaxy presents a relatively smooth morphology, suggesting an elliptical classification or a spiral seen face-on with a dominant bulge. The color profile indicates a population of older stars, with a yellowish-orange hue concentrated towards the core. The galaxy appears moderately luminous, with a compact central region. There's a slight elongation or cigar shape, but primarily the galaxy appears fairly circular. There are no visible signs of major disturbances such as tidal tails or strong asymmetries, and no merging events are immediately apparent. The outer regions of the galaxy fade gradually, without a sharp cutoff. The galaxy appears to be fairly quiescent with a low star formation rate.