The galaxy presents a morphology consistent with a spiral type, although the resolution limits precise classification. The galactic disk is inclined relative to our line of sight. Spiral arms are present. There is a color gradient, with the central bulge exhibiting a yellowish-white hue, indicative of an older stellar population. The outer regions of the disk appear bluer, suggesting ongoing star formation. Some asymmetry is present in the disk, potentially indicative of gravitational interactions or recent merger activity. Dust lanes are suspected within the spiral arms. A less luminous, irregular region is also evident, either merging or a region of intense star formation. The galaxy presents a moderate bulge. Some irregularities might indicate tidal features. The light distribution seems more clumped rather than smooth. 
