The galaxy presents as a central, luminous spheroid with a concentration of light towards the core, indicating a bulge morphology. The overall color profile suggests a combination of stellar populations; a yellow to white hue at the center may represent older, evolved stars, while the surrounding regions show a bluer tinge, suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy exhibits a degree of disturbance in its structure, hinting at possible past or ongoing interactions. There are no clear spiral arms, the morphology is more akin to an elliptical or lenticular galaxy. The galaxy shows moderate luminosity, indicative of a fairly substantial stellar mass. Overall, this galaxy appears to be undergoing active or recent star formation, with a substantial spheroid component and possibly a disturbed morphology.
