The galaxy presents as a somewhat elongated, spindle-shaped structure. The central bulge appears diffuse and shows a yellowish-orange hue, possibly indicative of an older stellar population. Fainter, bluer light extends along the major axis of the galaxy, suggesting the presence of younger stars or ongoing star formation regions, although these features are not particularly pronounced. The overall morphology appears relatively smooth, lacking prominent spiral arms or significant dust lanes. There is no clear evidence of a recent major merger event, although some minor distortions might be present in the outer regions. The galaxy appears to be relatively isolated, with no obvious interacting companions nearby.
