The galaxy appears to be an elliptical type, characterized by a smooth and featureless morphology. It exhibits a significant elongation, presenting a cigar-like shape. There is no visual evidence of spiral arms or a prominent disk structure. The galaxy has a concentrated central bulge region. There is no apparent ongoing merger activity or signs of significant tidal disturbances in its vicinity. The overall color profile indicates a population of older stars, with a redder appearance, suggesting a low rate of star formation.
