The galaxy presents as a somewhat elongated, disk-like structure, viewed at an oblique angle. There is a central bulge that appears quite prominent and concentrated, exhibiting a yellowish-orange hue. The outer regions of the disk are less defined, with a more diffuse and fainter appearance, exhibiting colors which tend towards blue. The smooth distribution of light suggests a relatively evolved system, though some subtle irregularities are present in the outer disk. There are no obvious signs of ongoing major merger activity, though some minor tidal disturbances cannot be ruled out given the image resolution. The overall color profile indicates a stellar population likely dominated by older stars in the bulge, with some younger, bluer stars contributing to the light in the disk. The galaxy is moderately luminous.
