The galaxy presents as a relatively compact object with an overall elliptical morphology. The light distribution appears smoother, with minimal evidence of spiral arms or distinct features within the main body. Its shape is more elongated than circular, tending towards a cigar shape. The color profile suggests a population of older stars, with a higher concentration of redder hues throughout the galaxy, although there are also some localized areas exhibiting bluer tints, possibly indicative of younger stellar populations or ongoing star formation. There is evidence of minor disturbance of the galaxy.
