The galaxy presents as a relatively smooth, elongated structure. Its overall shape is somewhat flattened, appearing cigar-shaped. The central region exhibits a bright, concentrated luminosity that appears to be a spheroid, possibly indicating the presence of an older stellar population. The surrounding regions display a gradient of decreasing light intensity, transitioning from a pale white-blue hue near the center to a faint and patchy blue-green in the outer regions. There is little to no evidence of distinct spiral arms, strong dust lanes, or significant irregularities in its form. The galaxy's appearance suggests a low level of ongoing star formation activity, concentrated primarily in the disc. There is no indication of a major merger event, although minor disturbances cannot be ruled out.
