The galaxy presents as a centrally concentrated, ellipsoidal system with a smooth, diffused light profile. The core region exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Moving outward from the core, the color transitions into a bluer tone. This suggests ongoing star formation or the presence of a younger stellar population in the outer regions. The overall structure appears undisturbed, with no obvious signs of tidal tails or ongoing mergers. There are some vague features that suggest the presence of a disk. Based on the color and morphology, it appears to be an intermediate-mass galaxy. The galaxy has a measured redshift, indicating its distance and the expansion of the universe at its location. The data collected on this object suggests this galaxy has a low star formation rate.
