The galaxy presents a predominantly smooth morphology with a subtle, but perceptible, deviation from a perfect elliptical shape. Its overall form appears slightly elongated. The central region exhibits a concentrated luminosity, suggesting the presence of a galactic nucleus. The light distribution appears fairly uniform across the galaxy, with a gradual decrease in brightness as one moves from the center toward the outer regions. The color profile appears to be redder in the central region, suggestive of an older stellar population, with a subtle shift towards bluer hues in the outer edges. There's also some evidence of minor disturbances. Though it may be due to image artifacts, these disturbances suggest that this galaxy may have recently undergone, or is currently undergoing, a minor interaction with another galaxy. This conclusion however is not definitive.
