The galaxy presents as a relatively smooth, elliptical morphology. It appears to be a concentrated spheroid of light, with a notable lack of defined spiral arms or a prominent disk structure. The light profile suggests a centrally concentrated distribution of stars. The central region exhibits a yellowish hue, potentially indicating an older stellar population. Moving outwards from the core, the galaxy’s color profile gradually transitions to a slightly redder tone, which could be caused by a gradual change in stellar age. It is not perfectly round; some elongation is detectable. There is no obvious evidence of any ongoing major mergers or significant tidal disturbances. The galaxy appears fairly isolated and undisturbed. Overall, this galaxy looks like an elliptical galaxy at an approximate distance corresponding to a redshift of roughly 0.066.
