The galaxy presents as a spiral type, observed at a slight angle relative to face-on. A central bulge is prominent, exhibiting a bright, concentrated luminosity suggesting a high stellar density within the nucleus. The bulge is more luminous than the disk, implying it may be a larger and more massive bulge.

The spiral arms are moderately defined, with a noticeable winding pattern, tracing a fairly symmetric structure. They appear somewhat flocculent, lacking continuous, well-defined segments. The color suggests a mix of stellar populations with the spiral arms, although the resolution limits a detailed analysis.

There appears to be an absence of a clear bar structure within the central region of the galaxy. The disk exhibits a relatively smooth appearance, but does have features like a bulge and spiral arms, indicating this is a relatively evolved system undergoing active star formation. Some minor asymmetrical features are present in the outer disk.
