The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless structure. The luminosity profile shows a strong central concentration, suggesting a significant bulge component. The overall color appears to be slightly redder, indicating an older stellar population compared to actively star-forming galaxies. There is no discernible evidence of spiral arms or a prominent disk. The galaxy appears relatively isolated, with no obvious signs of interaction or ongoing merging activity. The roundness of the galaxy's shape is moderate; it appears neither perfectly spherical nor significantly elongated. Based on these characteristics, the galaxy is likely a passively evolving elliptical galaxy.