This galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated luminosity profile. Its shape is somewhat elongated, more akin to a flattened spheroid than a perfect circle. It presents a yellow-white hue, indicative of an older stellar population with relatively little ongoing star formation. There are no distinct spiral arms or prominent dust lanes visible. No significant tidal features or morphological disturbances suggest a recent major merger, although some minor irregularity cannot be ruled out. The general morphology suggests a galaxy dominated by evolved stars and with a relatively high mass, where the rate of new star formation is low.
