The galaxy presents as an elongated structure, suggestive of a disk galaxy viewed at an oblique angle. A bright, relatively compact central bulge is evident, appearing somewhat spheroidal in shape and dominating the galaxy's luminosity. The disk component appears relatively smooth, with a subtle bluish tint, which may indicate the presence of younger stellar populations and ongoing star formation. Faint and patchy spiral arms, likely tightly wound, seem to emanate from the central region. No significant dust lanes or prominent star-forming regions are visible within the disk. The overall structure suggests a morphological type of late-type spiral galaxy exhibiting characteristics somewhere between Sa and Sb. Evidence of minor interaction or disturbance is noted on the periphery, hinting at a possible past or ongoing gravitational interaction. The light profile appears to be consistent with a centrally concentrated mass distribution, with a gradual decline in brightness towards the outer regions.
