The galaxy presents a diffuse, elliptical morphology with a relatively smooth profile. The central region exhibits a concentrated luminosity, transitioning into a less dense, extended halo. The galaxy appears predominantly yellow-orange in color, suggesting an older stellar population with lower rates of current star formation. Some subtle irregularities and minor disturbances appear to disrupt the general smoothness of the galaxy. There is also a faint bluish arm of material extending from the top center of the galaxy. These disturbances may be evidence of a past merger event. Overall, the system is moderately compact and appears to be in a transitional state between a spiral and elliptical galaxy, as there are remnants of both structures.