The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a high stellar density, possibly indicative of an aging stellar population. Moving outwards, the luminosity gradually decreases, with a faint, extended halo visible. There is a slight deviation from perfect ellipticity, leaning towards a somewhat oblate spheroid shape. No distinct spiral arm structures or prominent dust lanes are discernible, furthering the classification as likely an elliptical or lenticular galaxy. Subtle color gradients are observable, with the central region exhibiting a yellower hue, potentially resulting from older stars, while the outer regions appear slightly bluer, perhaps due to the presence of younger stars or ongoing star formation, though not particularly pronounced. There are no clear signs of ongoing major merger activity, although a slight asymmetry could indicate a minor interaction or disturbance.
