The galaxy presents as a spiral type, exhibiting a relatively well-defined disk structure. The spiral arms appear tightly wound, originating from a central bulge region that is moderate in size and exhibits a yellowish hue, suggestive of an older stellar population. The disk displays a bluer color, indicative of ongoing star formation within the spiral arms. Although a bar structure is suggested, it does not appear to be extremely distinct. There is no strong indication of a major merger event, though the overall morphology hints at potential minor disturbances, possibly from previous interactions.
