The galaxy presents as a centrally concentrated, elliptical-shaped object. Its light distribution is dominated by a smooth, diffuse component. There appears to be a distinct lack of spiral arm structures. The color profile indicates a generally red population, with the central region appearing yellower than the outskirts. This color suggests an older stellar population dominating the light output. There is no apparent dust lane or recent star formation activity visible in this image. The galaxy exhibits a high degree of central light concentration. Overall, the morphological characteristics align with that of an elliptical galaxy.
