The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears elliptical in shape, exhibiting a slight elongation but approximating a round structure. The color profile suggests a dominant red or yellow hue in the central region, transitioning outwards to a less saturated, greener halo. There is no apparent spiral structure or prominent disk component. The smoothness of the light distribution indicates the possible lack of recent major mergers, but the slight asymmetries may be due to minor disturbances. There are no immediately obvious signs of ongoing major star formation activity based on the color and morphological characteristics. The lack of distinct tidal features further supports the conclusion that this is not a recent major merger remnant.
