The galaxy presents as an elongated, cigar-shaped structure. Its color profile suggests a dominant redder hue, possibly indicating an older stellar population. There appears to be a smooth and relatively featureless light distribution across the galaxy's body. The overall structure appears largely undisturbed, with no obvious signs of major tidal interactions or significant ongoing mergers. There may be some indication of a very minor disturbance or internal structure within the galaxy, however the spatial resolution does not permit a more detailed morphological assessment. The galaxy's luminosity profile suggests it is a relatively massive system, with an appreciable star formation rate, though the system does not have the bluer color typically indicative of much higher levels of recent star formation.
