The galaxy appears to be a spiral galaxy viewed at a relatively slight angle. A bright central bulge is visible. The disk appears somewhat disturbed or flocculent, with hints of spiral arm structure but no well-defined, grand design spiral arms. The color of the central bulge is more yellow/red, which may indicate an older stellar population or a high amount of dust obscuration. The disk appears somewhat bluer, potentially indicating ongoing star formation. There may be faint tidal features or minor disturbances suggesting a past or ongoing interaction with another galaxy, though this is not conclusive from the image alone. The overall morphology is consistent with a galaxy that is neither a perfectly smooth elliptical nor a highly ordered spiral, but rather something in between, possibly an intermediate spiral type.
