The galaxy presents as a centrally concentrated object with a relatively smooth, diffuse appearance. Its color profile suggests an older stellar population, exhibiting a yellowish-white hue with a slight color gradient that becomes slightly redder towards the outer regions. There are no discernible spiral arms or distinct morphological features characteristic of younger, disk-dominated galaxies. The overall shape is moderately elliptical, with a slight deviation from a perfectly circular form. There is no evidence of strong tidal interactions or major disturbances, indicating it is likely not undergoing a major merger. Slight asymmetry may be present in the outer halo suggesting minor gravitational interaction.
