The galaxy presents a generally smooth morphology, with a spheroidal shape and no immediately apparent spiral arm structure. The central bulge region appears quite prominent and relatively bright, exhibiting a concentrated luminosity. The overall color profile suggests an older stellar population, skewed towards redder wavelengths, although there is subtle evidence of bluer components indicative of recent or ongoing star formation activity within the disk. There is a possible minor distortion in the outer regions, suggesting a past interaction or minor disturbance, but no signs of a major merger. The galaxy's shape appears round, lacking a highly elongated or cigar-like appearance. The overall structure suggests a galaxy which has largely completed its assembly, but remains moderately active in terms of star formation.
