The galaxy presents as a moderately inclined spiral, potentially nearing edge-on orientation. A prominent central bulge is observed, exhibiting a yellowish hue suggesting an older stellar population. Faint, diffuse disk is present with hints of bluer regions, possibly indicating areas of ongoing star formation. The structure of the arms is not well-defined, appearing somewhat flocculent, but the object does not appear to be undergoing a major merger or significant tidal disruption, rather a slight asymmetry. The object may be a relatively high-mass galaxy with a moderate rate of star formation.
