This galaxy exhibits an elliptical morphology, with a smooth, diffuse light distribution. The central bulge appears bright and concentrated, surrounded by a fainter, more extended halo. There is evidence of a slight disk component. The disk is inclined relative to our line of sight. The major axis is oriented at an angle of approximately 55 degrees relative to the horizontal axis of the image. The dust content appears minimal. Overall, the galaxy appears relatively undisturbed, showing no strong signs of recent major merger activity. The color suggests a population of older stars, contributing to the galaxy's redder appearance, but there is also blue-ish light distributed throughout the galaxy, potentially due to the presence of young stars.
