The galaxy presents as a somewhat elongated structure with a concentrated central bulge exhibiting a yellowish hue. Surrounding this core is a more diffuse disk-like component, displaying a subtle bluish color. This indicates ongoing, albeit possibly subdued, star formation activity within the disk regions. The overall morphology suggests a galaxy transitioning towards a lenticular or early-type spiral classification, with a moderately flattened shape and arm structures that are not well-defined. There is evidence of minor disturbances in its structure. The galaxy exhibits an elliptical profile, with an estimated effective radius of approximately 5 kiloparsecs.
