The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The core region exhibits a bright, yellowish hue, suggesting an older stellar population. Fainter, diffuse bluish light surrounds the core, potentially indicating some level of recent or ongoing star formation in the outer regions, albeit at a relatively low rate. The overall shape is generally round but not a perfect circle. There is no evidence of strong spiral arms or significant tidal disturbances, suggesting a relatively isolated and quiescent system. The galaxy appears to be a large, massive system given its overall luminosity and extent. 
