The galaxy presents a largely featureless, smooth morphology, suggesting an elliptical classification. It appears highly rounded in shape. The color profile is indicative of an older stellar population with a dominant yellow hue. This is consistent with a galaxy where star formation rates are relatively low. There is no discernible evidence of spiral arms or significant dust lanes. There does not appear to be any major disturbance to its shape or structure, suggesting that no major merging events have occurred. The overall impression is of a galaxy with a substantial stellar mass.
