The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated distribution of light. The core is the most luminous region, displaying a yellowish-orange hue indicative of an older stellar population with lower levels of ongoing star formation. The light gradually fades towards the outer edges, suggesting a decreasing stellar density. No prominent features such as spiral arms, dust lanes, or tidal tails are discernible, further supporting an elliptical classification. The overall structure appears relatively undisturbed, with no obvious signs of recent merger activity or strong gravitational interactions. The galaxy subtends a small angular size, consistent with its redshift. 
