The galaxy presents a mostly smooth morphology, exhibiting an elliptical shape that is somewhat elongated, appearing cigar-shaped. There's a brighter, concentrated central region, likely a bulge. Moving outwards from the center, the galaxy gradually fades into a fainter halo. The color profile suggests the presence of older stellar populations, with light becoming slightly bluer towards the outer regions, possibly indicating some ongoing, albeit low, levels of star formation. There is no prominent disk structure visible, nor is there evidence of major disturbances such as tidal tails or a merger in progress, although subtle asymmetries are present.
