The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile appears concentrated towards the center, indicative of a high degree of central mass concentration. The overall color is yellowish-orange, implying an older stellar population with a lower rate of ongoing star formation, consistent with the observed redshift. The galaxy's shape is elongated, cigar-shaped. There are no discernible spiral arms or prominent dust lanes, suggesting a lack of significant recent merger activity or gas accretion. The galaxy exhibits a redder hue compared to other field objects, supporting its classification as an evolved system with a reduced presence of young, blue stars. Overall, the observed features align with characteristics of a lenticular or early-type spiral galaxy at an intermediate redshift.
