The galaxy presents a predominantly smooth morphology, with a noticeable central bulge. The light distribution suggests a spheroid-like structure, with a gradual decrease in luminosity from the core outwards. The overall color appears relatively red, indicating a population of older stars and potentially a lower rate of active star formation. The shape is neither perfectly round nor elongated, but rather falls somewhere in between. There is no obvious evidence of major disturbances or ongoing mergers in the galaxy's structure, although a slight asymmetry cannot be entirely ruled out. The galaxy appears relatively isolated in this field, with no clearly interacting companion galaxies in close proximity.
