The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears elliptical in shape, lacking any obvious spiral arm structures. The core region is bright, transitioning to a fainter, more diffuse halo. There may be a very slight asymmetry to the overall shape. The color gradient indicates a population of older stars, suggesting a relatively low rate of current star formation. There is no evidence of any major ongoing merger activity. The galaxy appears undisturbed. 
