The galaxy presents a smooth morphology, characterized by a dominant spheroid shape. It appears elongated, with an approximate cigar-like form. There is no clear evidence of spiral arm structure or a prominent central bar. The galaxy displays a generally uniform color distribution, with a slight reddening towards the core and a subtle bluing in the outer regions, which could be indicative of differing stellar populations and activity across the galaxy. The galaxy is not obviously interacting with any other galaxies, although a very close inspection might reveal minor disturbances or asymmetries within the galaxy’s structure. The color and smoothness suggest a significant population of older stars and a relatively low rate of ongoing star formation.
