This galaxy exhibits a morphology that appears to be relatively smooth and elliptical in shape, though a slight disky component might exist. The central region presents a bright, concentrated core, potentially indicating the presence of an active galactic nucleus or a dense stellar population. Fainter, less defined regions extend outwards from the core, with a subtle color gradient visible, suggesting variations in stellar populations or dust content. There is a lack of spiral arm structure or strong star-forming regions, which would align with a galaxy with an older stellar population and less ongoing star formation. While seemingly isolated, there is very slight evidence of possible minor gravitational interactions, or a tidal feature that could be indicative of past interactions.
