The galaxy presents as a moderately luminous, concentrated object with a generally smooth morphology. There is a slight elongation and deviation from perfect circularity. The light distribution appears relatively even across the galaxy's body, with no prominent spiral arms or distinct features immediately apparent. A color gradient is discernible, with the central regions exhibiting a somewhat redder hue compared to the bluer outer edges. No signs of ongoing major merger activity are visually detected, though subtle disturbances or minor interactions cannot be entirely ruled out at this resolution. The galaxy's overall appearance suggests a relatively evolved system, possibly an elliptical or lenticular galaxy.
