The galaxy appears as a centrally concentrated object, exhibiting a largely smooth morphology. There is minimal evidence of spiral arm structures or prominent dust lanes. The light distribution is generally ellipsoidal, tending toward an intermediate roundedness. Some subtle, minor irregularities are present but do not point toward ongoing major mergers, nor are there any signs of tidal tails or shells. The object shows a yellow hue, indicating an older stellar population and suppressed recent star formation.
