The galaxy presents a generally smooth, rounded morphology. Its light profile appears centrally concentrated, with a gradual decrease in surface brightness moving outwards. The galaxy lacks any readily discernible spiral arm structure or a prominent galactic bar. There is no clear evidence of ongoing major mergers or significant tidal disturbances; however, a minor perturbation or interaction cannot be entirely ruled out. The galaxy exhibits a relatively uniform color profile, hinting towards a well-mixed stellar population and/or a lack of significant dust obscuration. The observed color suggests the presence of evolved stars with moderate star formation. The spatial extent of the galaxy appears compact, implying a relatively small physical size.
