The galaxy presents as an elliptical or lenticular system, exhibiting a relatively smooth morphology with a high degree of central concentration. A discernible bulge component dominates the central region, characterized by a yellowish-white hue, likely indicating an older stellar population. Fainter blue tinges extending outwards suggest a weak disk component with some on-going star formation. Subtle irregularities in the outer regions may indicate minor gravitational interactions or accretion events. The object appears to be reasonably massive and undergoing a period of modest star formation.
