The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless with no discernible spiral arms or bar structure. The light profile is centrally concentrated, exhibiting a bright, yellowish core, with a gradual decrease in intensity towards the outer regions. The color suggests an older stellar population, dominated by evolved, redder stars. The isophotes are mostly round, with a slight elongation indicative of a moderate ellipticity. There is no evidence of any major ongoing mergers or significant tidal disturbances, although a very slight asymmetry in the outer regions cannot be ruled out without deeper imaging. The overall appearance suggests a relatively quiescent system, with a low current star formation rate.
