The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. It presents an elliptical-like shape, showing high levels of apparent roundness. The central region displays a bright, yellowish hue, indicative of an older stellar population. Moving outward from the center, the color gradually transitions to a bluer tint, suggesting the presence of some younger stars within its outskirts. No distinct spiral arms or bar structures are discernible. The galaxy appears relatively isolated, exhibiting no prominent tidal features or signs of ongoing major merger activity, although the possibility of minor disturbances in the recent past cannot be entirely ruled out. The galaxy’s light appears to be redshifted and diminished by distance.
