The galaxy presents an elliptical morphology with a somewhat smooth appearance. It exhibits a concentrated central bulge with an apparent lack of significant spiral arm structures. The galaxy's color profile indicates a population of older stars, suggesting a relatively low current star formation rate. There is a subtle asymmetry to the galaxy's shape with a possible minor disturbance on one edge, this could possibly be explained by a minor interaction with a smaller nearby object or just a small pocket of star formation. Overall, the galaxy appears to be a relatively evolved system, likely situated at a cosmological distance.
