The galaxy appears as an elliptical-like structure. The object exhibits a relatively smooth morphology, with a centrally concentrated luminosity profile. The galaxy shows a yellowish hue, suggesting an older stellar population with lower levels of ongoing star formation. Its shape is more in between round and elliptical than highly elongated. There are no apparent signs of tidal disturbances or recent major mergers, indicating it is likely a relatively isolated system that has evolved without significant external interactions. The light suggests a redshift where we can study it but there are no clear, distinctive spiral arms or prominent dust lanes visible, pointing toward the smooth distribution of stars.