The galaxy presents as a moderately inclined spiral or lenticular galaxy. It appears to have a central bulge that is slightly elongated. The overall color profile indicates an older stellar population dominating, shifting towards redder wavelengths, with the central region exhibiting a more pronounced yellow-orange hue suggestive of aging stars. The outer regions of the galaxy show bluer colors, which may indicate some ongoing star formation, but this is not particularly prominent. There's a slight asymmetry to the outer regions of the disk, but no strong tidal features or indications of a recent major merger. The overall structure suggests a well-formed, relatively relaxed system in a later stage of its evolution.
