The galaxy presents as a relatively smooth, elliptical-like object. It displays a soft, diffuse glow with a slightly brighter core, but without any distinct spiral arm structures or prominent dust lanes. The galaxy appears to have a moderate ellipticity, leaning more towards a rounded shape rather than an elongated, cigar-like form. There are no visually apparent signs of ongoing major mergers or significant tidal disturbances; any interactions are likely minor or subtle. The color profile indicates an older stellar population with a lower rate of star formation. 
