This galaxy presents as an elongated, cigar-shaped system, likely an elliptical or lenticular galaxy seen at an oblique angle. The light distribution is concentrated towards the center, forming a bright nucleus or bulge region, which appears yellow-white in color, suggesting an older stellar population. The outer regions exhibit a diffuse, less defined structure with a gradual color shift towards redder hues, indicating a mix of stellar populations, potentially dust or older stars. There is no clear evidence of spiral arm structure or significant star-forming regions. No interactions or major disturbances are apparent in the immediate vicinity of the galaxy. Overall, the galaxy appears to be relatively smooth and undisturbed, indicative of a dynamically relaxed system.
