The galaxy presents as an elongated, spindle-shaped structure. It appears relatively smooth, with a notable absence of prominent spiral arms or distinct features that would indicate ongoing major disturbances or a recent merger event. The color gradient suggests a central bulge region that is comparatively redder, possibly indicative of an older stellar population. Moving outwards from the central bulge towards the edges of the galaxy, there's a shift towards bluer hues, which could signify more active star formation in those regions. The overall form is suggestive of a disk galaxy viewed at a high inclination angle, close to edge-on.
