The galaxy presents as a spiral type, viewed at a moderate inclination. A distinct disk structure is apparent, with a noticeably bright, somewhat elongated central bulge. Spiral arms are present, displaying a relatively tight winding pattern. The number of arms is difficult to precisely ascertain, but there are likely two to four arms. The disk exhibits variations in color, with bluer regions indicating areas of potential active star formation. There is no evidence of a major interaction or ongoing merger, although some minor irregularities or disturbances may be present within the disk. The central bulge appears yellowish, likely composed of an older stellar population. A weak bar structure is potentially present, though not clearly defined. The galaxy displays a generally ordered and symmetrical structure.
