The galaxy presents as a relatively compact object with an overall smooth morphology. The light distribution appears centrally concentrated with no obvious spiral arm features or prominent disk structures discernible. The galaxy exhibits an elliptical shape, approaching circularity. There is a slight elongation, but no apparent tidal features or signs of significant ongoing merger activity are observed. The color appears to be primarily concentrated in the redder wavelengths, suggesting an older stellar population and a low rate of current star formation. No distinct dust lanes or regions of active star formation are clearly visible within the galaxy's structure.
