The galaxy presents as a somewhat diffuse, elliptical object. It is characterized by a relatively smooth light distribution, with a bright central core that gradually diminishes in intensity towards the outer regions. The galaxy exhibits a subtle blue hue, suggesting the presence of a moderate population of young, hot stars. While the image quality limits detailed morphological assessment, there is a slight indication of minor disturbances or asymmetries in the outer regions, possibly suggestive of past or ongoing interactions. Overall, the galaxy appears to be an intermediate-mass system with a moderate amount of ongoing star formation and a mostly smooth, spheroidal morphology.
