The galaxy presents as an elongated, disk-like structure. Its central region displays a concentrated luminosity, exhibiting a yellowish-white color, suggestive of an older stellar population and reduced star formation. Moving outwards, the galaxy's disk appears to fade into a bluer hue, which may imply the presence of younger stars and active star formation. The overall structure indicates a lack of strong spiral arm definition and has a generally smooth appearance. There are some slight irregularities in the outer regions, however the galaxy is largely undisturbed. No clear signs of a major merger event are visible.
