The galaxy appears to be a luminous, early-type system at a moderate redshift. The galaxy core presents a smooth, centrally concentrated morphology, with a predominantly yellow hue, suggesting an older stellar population. There is a subtle extension of light outward from the center, indicative of a spheroidal component. Hints of redder, potentially dust-obscured regions are observed, although these do not significantly disrupt the galaxy's overall smooth appearance. The galaxy presents a relatively round shape, lacking any obvious spiral arms or strong tidal features, suggesting it is not currently undergoing a major merger. There are minor disturbances present, suggesting either a small tidal interaction or some sort of internal asymmetry.
