This galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The light distribution is dominated by older stellar populations, presenting a yellowish-red hue, indicative of lower levels of ongoing star formation. No distinct spiral arms or dust lanes are visible. The overall morphology suggests a system that is well evolved, potentially a result of past mergers or internal dynamical processes that have shaped its current form. There might be slight disturbances, possibly minor interactions with smaller companions. The galaxy's roundness suggests a low inclination angle relative to our line of sight.
