The galaxy appears as a centrally concentrated, elliptical or lenticular structure, exhibiting a smooth morphology with minimal discernible features such as spiral arms or a prominent disk. Its shape is approximately round. The color profile indicates a relatively red hue, suggesting an older stellar population and a low rate of ongoing star formation. There is no clear evidence of a major merger event. There may be some indication of minor tidal disturbances, but they are subtle. The galaxy is of moderate size and luminosity.