The galaxy presents as a lenticular or early-type spiral galaxy at a redshift of approximately 0.25. The central bulge appears relatively smooth and featureless, with a high degree of rotational symmetry. There is a slight elongation, suggesting a disk-like structure. Subtle features may indicate the presence of faint spiral arms or tidal disturbances, however no definitive arms are present. The color profile indicates a population dominated by older stars, with minimal evidence of ongoing star formation. The overall light distribution is concentrated towards the center, indicative of a well-established stellar population. There is a hint of a fainter, extended halo surrounding the main galactic body.
