The galaxy presents a largely smooth morphology. It appears elliptical or lenticular with a dominant central bulge. There's an absence of prominent spiral arms or a well-defined disk structure. The light distribution is concentrated towards the center, suggesting an older stellar population. The galaxy exhibits a high degree of symmetry, with an absence of significant tidal features or distortions that might indicate recent interactions or mergers. Color gradients are subtle but present, with the central regions appearing somewhat yellower than the outer edges, consistent with an increase in older stars toward the nucleus. Based on its appearance, this system is likely an early-type galaxy, possibly an elliptical or an S0 type, with little ongoing star formation.
