The galaxy presents as a slightly elongated structure with a distinct central bulge. The core exhibits a concentrated luminosity, appearing a yellowish-orange hue, suggesting a population of older stars. Fainter, bluer extensions emanate from the main body, possibly indicating regions of more recent star formation. These areas appear less defined and more diffuse. The overall morphology suggests a classification somewhere between an elliptical and a spiral galaxy, potentially an S0 type. There appears to be a second, rounder object close to the edge of the galaxy, which could be another smaller galaxy or simply a region of intense star formation. There is some indication of tidal disturbance.
