The galaxy presents as a single, concentrated light source. The overall morphology appears largely smooth, with a slightly elongated, almost elliptical shape. The light distribution is centrally concentrated, with a bright core that diffuses outwards. There's a noticeable color gradient, shifting from a bluer hue at the center to a more reddish tint in the outer regions. This could indicate a difference in stellar populations, with younger, bluer stars dominating the core and older, redder stars residing in the outer regions. There is no clear evidence of spiral arms or a distinct disk structure. There is also no obvious sign of a major merger or tidal disturbances.
