The galaxy presents as an elongated, likely elliptical or lenticular system. Its central bulge appears concentrated with a yellow-orange hue, indicative of an older stellar population. Extending outward from the core, we observe a fainter, bluer disk. The blue color indicates ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major merging events, though there is a slight asymmetry in the outer regions, suggesting a possible minor interaction or past disturbance. Overall the galaxy has a smooth appearance, with a high degree of central concentration.
