The galaxy presents as a relatively smooth, elliptical-like structure with a bright central core. There is a noticeable radial decrease in luminosity from the center outwards, indicating a concentration of stellar density towards the nucleus. The galaxy appears slightly elongated but generally spheroidal, leaning toward an in-between roundness. There is no apparent indication of ongoing major mergers or significant tidal disturbances. Faint, diffuse outer regions suggest a halo of stars extending beyond the main body. The color profile appears relatively uniform across the galaxy, with a blueish hue indicating the presence of hot, young stars, or it could be a result of redshift. However, the dominant morphology implies an older stellar population. Star formation appears minimal. 
