The galaxy presents as a centrally concentrated object, exhibiting an overall smooth morphology. It is generally circular in appearance. There is some indication of a slight asymmetry or possible disturbance in the galaxy's outer regions, though this could be due to image artifacts or faint tidal features. Color gradients suggest a possible variation in stellar populations or dust content across the galaxy, with a somewhat bluer hue in what may be a fainter and smaller disk-like structure in the central regions. Overall the galaxy is quite red, indicating an older stellar population and suppressed recent star formation. The luminosity profile seems to be centrally peaked, suggesting that this galaxy is a spheroidal or elliptical galaxy. There is little evidence of spiral arm structure or significant dust lanes within the image.
