The galaxy exhibits an overall elliptical morphology, appearing elongated across the field of view. Its central region is characterized by a bright, concentrated light distribution, suggesting a relatively dense stellar population. The light profile appears smooth and generally featureless across the galaxy. A faint disk may be present; however, any discernible features are subtle and lack a defined spiral structure. There is no strong evidence of major mergers or significant tidal disturbances in the immediate vicinity. The galaxy appears relatively isolated and unperturbed. A slight asymmetry exists in the light distribution, possibly hinting at a minor interaction or internal dynamical process.
