The galaxy appears as a centrally concentrated object with a relatively smooth morphology. The core region exhibits a bright, somewhat diffuse glow, transitioning outwards to a less luminous halo. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The shape appears nearly circular, with minimal ellipticity. There is no obvious evidence of any ongoing major merger events or significant tidal disturbances. Faint and very subtle indications suggest the possibility of very minor disturbances in the outer regions of the galaxy. The color profile shifts slightly from a somewhat bluer hue in the outskirts to a yellower/redder hue in the central bulge, suggesting a possible difference in stellar populations.
