The galaxy presents an overall elliptical morphology, appearing somewhat elongated rather than perfectly spherical. The light distribution appears relatively smooth throughout the galaxy, with a concentration towards the central region, though subtle deviations suggest possible internal structures. Two brighter and concentrated regions seem to be present within the central area, suggesting either a double nucleus or intense star forming activity. The color profile indicates an older stellar population as a whole, with the central areas presenting a slightly bluer hue suggesting younger stars. It's hard to discern if this galaxy presents spiral arms or a prominent disk, but the elongated structure suggests a disk might be present or might have been perturbed. Indications of minor disturbances in its structure or the result of possible past merging activity are suggested.
