The galaxy presents as a relatively compact object with an apparent magnitude in the red band consistent with a distant source. The overall morphology suggests a relatively undisturbed system, lacking prominent tidal features or evidence of ongoing major mergers. There is some indication of disk or spiral-arm like features, yet they are not very prominent, it is very difficult to ascertain a classification of these features. The core of the galaxy appears fairly smooth, with a gradual fading of luminosity towards the outer regions. The color distribution appears relatively uniform across the galaxy, with a subtle reddening toward the central regions. There are very mild disturbances that may possibly be interpreted as potential minor merger events. Overall, the galaxy appears to be a moderately luminous, relatively isolated system with either weak spiral structure or no spiral structure.
