The galaxy presents as a relatively smooth, centrally concentrated object, appearing largely elliptical in shape. Its core region exhibits a bright, almost stellar-like concentration of light, suggesting a possible active galactic nucleus or a dense stellar population. The light gently fades from the center to the outer edges of the galaxy, with no distinct spiral arm structures visible, suggesting either a lack of prominent spiral arms or a viewing angle that obscures such features. A slight color gradient can be observed, with the central region exhibiting a more yellow hue transitioning to redder tones in the outskirts. No signs of major mergers or tidal disturbances can be identified in this image.
