The galaxy appears to be a relatively smooth, elliptical type. It exhibits a somewhat elongated shape, appearing slightly cigar-shaped rather than perfectly round. The central bulge region is prominent and displays a yellowish-orange hue, suggesting an older stellar population. Fainter, bluish regions are observed in the outer disk, hinting at the presence of some younger, star-forming regions, though the overall star formation rate appears moderate. There is no indication of major disturbances or ongoing mergers; the galaxy seems relatively isolated and undisturbed. The overall morphology indicates a galaxy that is likely transitioning towards a redder, quiescent state.
