The galaxy presents as a relatively smooth, rounded object. The color profile leans towards a yellowish-red hue, suggesting an older stellar population. No distinct spiral arms or bar structures are apparent in this image. The galaxy appears centrally concentrated with a gradual decrease in luminosity outwards. There are no visible signs of active galactic nuclei activity or significant dust lanes obscuring the central region. The morphology suggests a possible elliptical galaxy or a lenticular galaxy viewed face-on, with a high degree of symmetry and limited evidence of ongoing star formation. There is no indication of major mergers or tidal disturbances in the surrounding region.
