The galaxy presents a generally smooth morphology, though not perfectly elliptical. There is a slight disk-like structure, making it appear more like a lenticular galaxy than a pure elliptical. The color distribution shows a central concentration of yellow-orange hues, suggesting an older stellar population in the core, with the outer regions displaying bluer tints, hinting at the presence of younger stars and possibly ongoing star formation, although at a low rate. The galaxy appears relatively isolated with no obvious signs of major interaction, though a very minor disturbance or irregularity cannot be ruled out due to the galaxy's asymmetrical shape. The object appears somewhat rounded but is slightly elongated.
