The observed galaxy presents a predominantly smooth morphology. The primary body of the galaxy exhibits an elongated, cigar-like shape. There is a suggestion of some disturbance from smoothness with faint indications of asymmetrical features or faint disk-like structures embedded within the brighter central region. The central region of the galaxy appears brighter and more concentrated, with a diffuse glow extending outwards. The color profile suggests a population of older stars, based on the greater red color, although there is a distinct blue color. The galaxy does not display any obvious signs of a major merger event, but slight irregularities in the outer regions suggest a possible minor interaction or recent disturbance.
