The galaxy presents a notable spiral structure, although with relatively tightly wound arms. The central bulge appears prominent and exhibits a smooth, concentrated light distribution, suggesting a significant population of older stars. The spiral arms are somewhat flocculent, showing evidence of ongoing star formation through the presence of bluish regions, indicative of younger stellar populations. Dust lanes are subtly visible within the spiral arms, particularly on the near side of the galaxy. Overall, the galaxy appears to be relatively isolated and undisturbed, with no obvious signs of a major ongoing merger or tidal interactions with other nearby galaxies. It presents a generally smooth and continuous luminosity profile suggesting a relatively stable structure. The galaxy's light distribution is generally round, though slightly elongated.
