The galaxy exhibits a generally smooth morphology, with a notable absence of prominent spiral arm structures or irregular features. It presents an elliptical shape, appearing significantly elongated rather than spherical, trending toward a "in between" designation with slightly rounded features. The central bulge is bright and well-defined, with the overall color profile suggesting a population of older stars. This indicates a relatively quiescent star formation rate. There is no evidence of ongoing major mergers or significant tidal disturbances within the galaxy's structure. 
