The galaxy presents an elongated morphology, suggesting an elliptical or lenticular classification. Its light distribution is dominated by a smooth, centrally concentrated bulge. The color gradient appears redder toward the core, indicative of an older stellar population. Fainter, bluer light extending from the galaxy's main body hints at potential low-level star formation, likely distributed across the galaxy. The isophotes are generally regular, though subtle disturbances are noticeable, particularly along the major axis, which may be indicative of past minor merger events. No prominent spiral arm structure or dust lanes are apparent. Based on its apparent color, size, and lack of distinct morphological features, this galaxy appears to be a relatively massive system at a non-negligible redshift.
