The object presents as an elliptical galaxy, viewed at an angle that is moderately inclined relative to our line of sight, giving it a somewhat elongated, cigar-shaped appearance. The light distribution is smooth and centrally concentrated, with the highest intensity appearing at the core, suggesting a significant bulge component. There is a subtle color gradient, with the central region exhibiting a slightly yellower or whiter hue, possibly indicative of an older stellar population or dust obscuration. The outer regions of the galaxy appear bluer, suggesting the presence of some younger stars or ongoing, though possibly low, star formation. There appears to be no obvious evidence of spiral arm structure or major disturbances in the galaxy's morphology, though there may be a minor asymmetry in the distribution of light, hinting at a possible past minor interaction or merger. Overall, the object is consistent with a relatively massive galaxy at an intermediate redshift with a moderate level of star formation.
