The galaxy presents a generally smooth, elliptical morphology, with a slightly elongated shape. There is a concentration of light towards the center, suggesting a prominent bulge. While a detailed analysis of internal structure is limited by image resolution, there does not appear to be strong evidence of spiral arms or distinct disk features. Based on its color, this galaxy appears to be a relatively mature system, with a substantial population of older stars. There appears to be no major interaction with other galaxies and no significant disturbances.
