The galaxy presents as a somewhat elongated, disk-shaped structure with a bright, concentrated central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the bulge, there's a fainter, bluer disk component, indicative of more recent star formation. The disk's morphology is not perfectly smooth; there appears to be some texture, with hints of spiral arm structures or patchy regions of star formation. There is a subtle warping or minor disturbance of the morphology, suggesting the possibility of an interaction or past merger event. The galaxy appears relatively isolated in the field of view.
