The galaxy appears as a moderately elongated structure. Its central region exhibits a smooth, concentrated light distribution, suggestive of a significant bulge component. The outer regions show a fainter, more diffuse glow, possibly indicating a disk. There is no apparent spiral structure. The overall color suggests a population of older stars. There is possibly a very small merger visible to the side, indicating some disturbance of the galaxy. The galaxy is of significant size and mass, possibly an early-type galaxy. Star formation appears to be somewhat quiescent.
