The galaxy presents as a somewhat amorphous structure, exhibiting a dominant, smooth morphology with an elliptical appearance. There is little evidence of spiral arms or a distinct disk-like structure. The light distribution is concentrated towards the center, suggesting a bright central bulge or core. The radial color gradient suggests a population of older stars towards the center with the outskirts appearing bluer. The galaxy is not perfectly round, displaying an overall elliptical profile. No significant tidal tails or signs of a major merger are discernible. There is a suggestion of some minor perturbation or interaction present in the outskirts of the galaxy, and low-level star formation activity may be occurring. The galaxy is moderately luminous.
