The galaxy appears to be a large, relatively smooth system with a prominent central bulge. The light profile suggests a concentration of older stars in the core, exhibiting a yellowish-orange hue.  The galaxy appears somewhat elongated, neither perfectly spherical nor disk-like. There are faint indications of diffuse, extended features or tidal tails suggesting some interaction or past merger event, although this is not a strong visual component. No distinct spiral arms or features of active star formation are observed in the image. Overall, the galaxy presents an elliptical or lenticular morphology with a possible minor interaction.
