The galaxy appears to be a spiral galaxy, viewed at an oblique angle, with an estimated redshift of approximately 0.046. There is evidence of well-defined spiral arms emanating from a central bulge, which appears to be of moderate size. The spiral arms exhibit a bluer color, potentially indicating regions of active star formation. Dust lanes are faintly visible along the inner edges of some spiral arms. The overall morphology suggests a galaxy with ongoing star formation and a relatively well-defined disk structure. There is no strong evidence of a bar structure, but the central region appears somewhat elongated. The galaxy does not appear to be undergoing a major merger, although there may be some minor tidal disturbances or interactions.
