This galaxy appears to be relatively smooth and elliptical in shape. There is a concentration of light towards the center, suggesting a well-defined nucleus or bulge. The galaxy exhibits a somewhat uniform color distribution, with a slightly redder hue, particularly noticeable toward the core. The lack of prominent spiral arms or dust lanes suggests this is likely an early-type galaxy, potentially an elliptical or lenticular. There is evidence of a minor disturbance or interaction with a smaller object in the vicinity of the larger galaxy, potentially another galaxy with bluer colors. This smaller galaxy has a more irregular morphology, possibly indicating ongoing star formation. The overall appearance suggests a galaxy that has undergone significant evolution, with a dominant older stellar population.
