The galaxy presents as a spiral type, displaying a prominent disk structure. Evident are well-defined spiral arms, exhibiting a moderate winding pattern. The arm structure has a relatively high degree of symmetry. Dust lanes are subtly visible along the inner edges of the spiral arms, but do not dominate the visual appearance. A central bulge is notable, exhibiting a moderate size in relation to the disk. The bulge appears relatively smooth and concentrated. The galaxy shows signs of a bar structure crossing the central bulge. The overall color is indicative of a mix of stellar populations. The central region appears yellower, suggesting older stars. The spiral arms show a bluer tint, potentially indicating younger stars and active star formation. There is no strong evidence of tidal disturbances or interaction with other galaxies, although subtle asymmetries in the outer disk could suggest minor past interactions. The galaxy’s morphology suggests it is a relatively isolated spiral galaxy undergoing ongoing star formation within its spiral arms.
