The galaxy presents as a single, centrally concentrated object with a smooth and relatively featureless morphology. The light profile appears diffuse, with a gradual decrease in intensity from the core outwards. The core region exhibits a yellowish-orange hue, suggesting an older stellar population and/or significant dust content attenuating bluer wavelengths. Fainter, diffuse extensions of light are visible surrounding the central region, potentially representing a halo or an extended disk component. There is minimal evidence of spiral arms or distinct substructures. The overall shape is somewhat elliptical, showing a deviation from being perfectly spherical. Indications of a potential minor disturbance can be seen within the light distribution. The galaxy appears to be relatively isolated, without any obvious signs of ongoing major mergers. Its color indices suggest that it's dominated by older stars, with minimal active star formation regions contributing to its overall luminosity.
