The galaxy presents as a concentrated, elliptical form. The light profile is smooth and centrally concentrated, with a gradual falloff in intensity towards the outer regions. The core exhibits a yellowish hue, suggestive of an older stellar population dominating the central region. The lack of distinct spiral arms or prominent dust lanes indicates a relatively quiescent system, perhaps a galaxy that has largely exhausted its gas supply for active star formation. The overall morphology suggests a system approaching a spheroidal shape, with little evidence of ongoing mergers or major disturbances. The galaxy’s size appears moderate, with a significant contribution from the central bulge component. The slight elongation suggests that it is more akin to an E4-E5 elliptical galaxy.
