The galaxy presents as a smooth, elongated structure. Its shape is reminiscent of a cigar, with a length significantly exceeding its width. The central region exhibits a bright, concentrated luminosity. This bright region transitions smoothly outwards, becoming less intense toward the galaxy's edges. There is evidence of a disk-like structure, though the smooth overall appearance suggests a dominance of older stellar populations. No major disturbances or merging features are apparent, indicating a relatively quiescent state. The galaxy’s color profile suggests moderate star formation activity, with the overall color appearing somewhat redder, indicating it is primarily composed of older stars.
