The object presents as an elliptical galaxy, exhibiting a generally smooth morphology with a high degree of central concentration. Its shape is largely circular. There may be a minor disturbance within the galaxy's structure, with some suggestion of interaction or merging activity; however, the dominant characteristic is a singular, cohesive form. The colour appears to be primarily redder, suggesting an older stellar population with relatively little ongoing star formation. Based on the colour profile, the stellar population is likely dominated by older, redder stars, indicative of a galaxy that has largely ceased star formation.
