The galaxy presents as a single, relatively smooth, centrally concentrated object. Its morphology is largely elliptical, appearing mostly round with a slight deviation toward a more elongated form. The central region exhibits a bright yellowish hue, suggestive of an older stellar population. Fainter, slightly bluer light extends outwards from the core, indicating regions of more recent or ongoing star formation, though limited. No significant spiral arm structures or major dust lanes are discernible. There is no evidence of major mergers or tidal disturbances.
