The galaxy presents as a roughly elliptical shape. The light distribution appears concentrated towards the center, with a bright, yellowish core indicative of an older stellar population or potentially an active galactic nucleus. Fainter, bluer light extends outwards from the central region. The object exhibits a disk-like appearance, with faint spiral arms visible. The galaxy's disk is tilted relative to our line of sight. There is no indication of a major merger in the recent past, although the slight asymmetry in the galaxy's shape might suggest minor tidal interactions or disturbances. The galaxy’s surface brightness appears relatively smooth. The color gradient suggests ongoing star formation, primarily occurring in the outer regions of the galaxy.
