The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, with a high degree of roundness in its isophotes. There are no prominent spiral arms or bar-like structures visible. A slight color gradient is observed, with the central region exhibiting a subtle reddish hue, potentially indicating an older stellar population. Fainter, bluer regions are observed in a small disk-like structure, indicating ongoing star formation. There are no signs of major mergers, though there may be a slight disturbance visible that suggests minor interaction with another object.