The galaxy presents as a slightly inclined spiral with a distinct disk structure. The central bulge appears moderately prominent, exhibiting a yellowish hue, indicative of an older stellar population. Spiral arms are discernible, emanating from the central bulge and displaying a bluer color, suggesting ongoing star formation within these regions. A slight asymmetry is noted in the arm structure, potentially indicating a minor gravitational disturbance or interaction. Dust lanes are vaguely visible, particularly along the inner edges of the spiral arms, obscuring some of the background starlight. The galaxy's overall shape is elongated, with a relatively high ellipticity.
