The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its morphology is largely elliptical or lenticular, exhibiting a round shape with a slight deviation toward an in-between, not perfectly circular form. There is a suggestion of a very faint, diffuse halo extending beyond the core region, though it is difficult to discern definitive structural features. The color profile suggests a population of older stars, exhibiting a redder hue centrally, implying the likelihood of a more evolved stellar population in the core and diminishing active star formation. There are no distinct spiral arms or bar structures visible, suggesting the galaxy is likely not a spiral type. The overall impression is of a relatively undisturbed system that is not undergoing any major merging events.
