The galaxy presents as a somewhat diffuse, elongated structure. It appears to have a central, brighter region which could be the galactic bulge, with fainter, extended arms or tidal features emanating from it. The color distribution indicates potential variations in stellar populations. The bluer hue observed suggests the presence of younger, hotter stars and active star formation regions, especially in the apparent tidal features. There is some evidence of a possible interaction or past merger event, as the galaxy's shape deviates from a typical elliptical or spiral structure. Irregularities and asymmetries in the light distribution further support this hypothesis. The galaxy is not strongly redshifted, indicating it is relatively nearby.