The galaxy presents as a centrally concentrated elliptical or lenticular system. The light profile smoothly decreases from the core outwards, exhibiting no obvious spiral arm structures or dust lanes. The core region appears to be the brightest and yellowest, implying a concentration of older stellar populations. The outer regions of the galaxy are more diffuse and redder in color, with the extreme edges fading significantly into the background. The galaxy is somewhat elongated, deviating noticeably from a perfectly circular morphology. There is no evidence of any significant tidal disturbances or ongoing major mergers. Based on the overall smooth morphology, and redder hue, it is likely this galaxy has a smaller star formation rate than galaxies of similar size that feature spiral structures.
