The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile appears predominantly blue-white, suggesting a population of younger, hotter stars. There are no immediately obvious spiral arm structures or significant dust lanes visible. The galaxy exhibits an elongated shape, leaning towards a cigar-like morphology. There are no prominent signs of ongoing major mergers or tidal disturbances, but some minor irregularities in the outer regions cannot be ruled out. The galaxy's overall structure indicates that it may be a relatively quiescent system with low star formation rates.
