The galaxy appears to be a relatively smooth, elliptical galaxy. Its shape is elongated, with a cigar-like appearance, exhibiting a clear major axis. The central bulge is prominent and smoothly blends into the outer regions, showing no distinct features like spiral arms or a bar. The light distribution indicates a concentration of older stellar populations, as evidenced by the reddish hue of the central region. There's minimal evidence of dust lanes or active star formation regions. The galaxy appears isolated, with no obvious signs of ongoing or recent merger activity. The galaxy's overall structure suggests it is a spheroidal system dominated by an older stellar population, residing within the 'red sequence' of galaxies.
