The galaxy appears to be elliptical, displaying a largely smooth morphology with minimal discernible features, such as spiral arms or prominent dust lanes. The overall shape appears relatively round. There is little evidence of ongoing or recent major mergers or tidal disturbances. Color gradients are subtle, with the central region exhibiting a slightly yellower hue, possibly indicative of an older stellar population or dust concentration. The galaxy’s light profile suggests a centrally concentrated luminosity, which is characteristic of elliptical galaxies. There is no obvious presence of substantial star formation activity based on color. 
