The galaxy appears to be a relatively compact, elliptical system. The central region exhibits a high concentration of light, appearing yellow-orange in color, suggesting an older stellar population. Moving outward from the core, the light intensity decreases gradually, transitioning to a more diffuse, bluer hue in the outer regions. This suggests the presence of some younger stars, although these appear to contribute less significantly to the overall luminosity than the core population. No distinct spiral arms or bar structures are visible. The galaxy presents a smooth overall appearance, but there are some hints of minor disturbances or tidal features at the edge. The shape is generally round, and it does not obviously appear to be in the middle of a merger event.
