The galaxy presents a generally smooth morphology, with a high degree of central concentration. The overall shape is elliptical, exhibiting a somewhat rounded appearance. The color profile leans towards the redder end of the spectrum, indicative of an older stellar population. There is no discernable spiral structure or prominent dust lanes. The galaxy appears to be relatively undisturbed, showing no obvious signs of recent or ongoing major mergers or tidal interactions, although minor disturbances cannot be ruled out. Based on the observed color and morphology, this galaxy likely has a low rate of star formation and a high stellar mass.
