The galaxy presents a generally smooth and rounded morphology, suggestive of an elliptical or lenticular type. Its color exhibits a reddish hue, potentially indicating an older stellar population with fewer young, massive stars. There is a faint asymmetry or minor perturbation in the galaxy's structure, possibly hinting at a past or ongoing interaction. No distinct spiral arms or bar features are discernible. The galaxy appears to have a concentrated core region, with light intensity gradually diminishing towards the outer regions. Overall, the galaxy's appearance is generally smooth and concentrated, suggesting a relatively evolved system.
