The galaxy appears to be a spiral type, though observed at an oblique angle, possibly approaching edge-on orientation. Prominent spiral arms are discernible, exhibiting a relatively loose winding pattern. Two main arms seem to dominate. A possible bar structure is suggested by the concentration of light towards the central region. The central bulge displays moderate size relative to the overall disk. Patches of bluer light are observed within the spiral arms, potentially indicating regions of active star formation. Overall, the galaxy's morphology suggests a disk galaxy undergoing moderate star formation. Evidence of a minor disturbance is present, perhaps due to a nearby interaction.
