The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical morphology with a concentrated central bulge. The light distribution suggests an older stellar population, with a yellow-red hue indicating the presence of evolved stars. There is little evidence of spiral arms or significant dust lanes, and no clear indication of ongoing major star formation. The galaxy is relatively compact, with a somewhat spherical shape. Any evidence of recent merger activity or tidal disturbances appears to be minimal.
