The galaxy presents a generally smooth and diffuse appearance with some apparent irregularities. There is a bright, concentrated central bulge or core, indicating a high density of stars in that region. The outer regions of the galaxy appear less defined, suggesting a gradual decrease in stellar density with distance from the center. There is some evidence of a possible disk-like structure although indistinct, indicated by the slight flattening along the horizontal plane. There appears to be evidence of an ongoing or past merger event, with a notable disruption of its smooth structure. The galaxy exhibits a reddish hue, suggesting a population of older stars, and a relatively low rate of ongoing star formation. There's subtle hint of bluer regions, near the nucleus but its presence is minimal. The overall luminosity suggests a massive galaxy. 
