The galaxy presents as a slightly elongated, diffuse object. Its core appears to be bright, with a relatively smooth, though not entirely uniform, light distribution emanating outwards. There is a subtle color gradient, transitioning from a brighter, bluer center to a more reddish hue in the outer regions. No distinct spiral arms or bar structures are readily apparent. There may be some subtle distortions in the overall shape of the galaxy, possibly indicating gravitational interaction. However, these possible disruptions appear to be minor in nature. The galaxy appears relatively isolated, without any immediately obvious companion galaxies or tidal features. 
