The galaxy presents as a relatively smooth, centrally concentrated structure with a slightly elongated morphology. The core region exhibits a bright, yellowish hue, suggestive of an older stellar population. Moving outwards from the core, a subtle color gradient towards bluer tones is observed, potentially indicating regions of more recent star formation, however these are not very pronounced. There are no clear spiral arm structures or prominent dust lanes visible. Minor disturbances are present but do not drastically impact the overall structure. Based on its general appearance, this galaxy appears to be an elliptical or lenticular galaxy at an intermediate redshift.
