The galaxy presents as a centrally concentrated spheroid with a smooth overall appearance. There is some faint structure and faint colors in the outer regions, but the general shape and the high central concentration suggests it's more elliptical than spiral. There may be some slight distortion visible, potentially indicating a minor interaction or disturbance but this is difficult to confirm given the image resolution. The galaxy exhibits a color gradient, with a bluer hue towards the outer regions, possibly indicating younger stellar populations there, and a central region that seems redder, indicating older stars. The galaxy appears fairly isolated, with no clear indication of nearby major companions or tidal features to suggest an ongoing or recent major merger. The lack of well-defined spiral arms or a prominent disk structure further supports a classification as a galaxy along the elliptical sequence.
