The galaxy appears as a centrally concentrated system with a flattened, elongated shape reminiscent of a cigar. There is a general lack of clear spiral arm structure. The central region presents a brighter, smoother appearance, while the outer regions show more diffuse and irregular characteristics. The color profile seems to indicate a mixture of stellar populations, with the inner regions exhibiting a slightly redder hue, potentially indicating older stars, and the outskirts displaying bluer tones suggestive of younger, star-forming regions. There is some indication of minor disturbances in its structure.
