The galaxy presents a generally smooth, elliptical morphology, appearing largely undisturbed. Its light profile suggests a centrally concentrated spheroid. The color distribution is not uniform, with a central region exhibiting a pinkish hue, potentially indicating ongoing or recent star formation or an older stellar population in the bulge. A subtle gradient of blue-green color extends outward from the central region, possibly attributable to a younger stellar population or dust. The galaxy is classified as likely non-merging with a generally spheroid shape.
