The galaxy appears as a luminous, elliptical structure. Its overall morphology suggests a relatively smooth distribution of light, with a high degree of central concentration. The core is bright and concentrated, exhibiting a yellowish hue which possibly indicates an older stellar population. Moving outwards from the center, the galaxy appears less dense and has a slightly bluer tinge. The shape indicates it is closer to 'in between' rather than perfectly round or cigar-shaped. There is no prominent evidence of spiral arms or significant dust lanes. There's no indication of major ongoing merger activity or strong tidal distortions. Overall it appears to be a large, relatively evolved galaxy with a moderate redshift and inferred high mass. Star formation activity is likely low.
