The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is no evidence of a strong spiral structure or bar. The color is largely uniform throughout, with a slight bluing toward the center and fading to a yellowish hue on the edges. The roundness indicates that the object is closer to spheroidal than disk-shaped. The galaxy's light is somewhat diffused, rather than sharply defined, potentially indicating a relatively high redshift. There is no sign of on-going major merger activity, although a slight asymmetry might suggest minor interaction. The overall appearance suggests a galaxy dominated by an older stellar population, but some indicators of on-going star formation might be present toward its center.
