The galaxy presents as a relatively smooth, centralized object. The overall color profile indicates a population of older stars, with a noticeable lack of distinct spiral arm structure or prominent dust lanes. There is a slight elongation in its shape, appearing somewhat oblate, but it is largely symmetrical. No distinct features are discernible in the image, suggesting either a quiescent state or internal processes that are not readily apparent at this resolution. There is no indication of active galactic nuclei activity or any ongoing major merger events. There is some minimal evidence of recent star formation. Overall, this galaxy likely falls into the category of an elliptical or lenticular galaxy with moderate mass and low star forming potential.
