The galaxy appears as a concentrated, elliptical shape with a smooth luminosity profile. The central region exhibits a bright, yellowish-orange hue, which gradually fades towards the outer edges. The galaxy appears elongated, with an aspect ratio indicating a cigar-like shape. There is no clear evidence of spiral arm structures or significant dust lanes. The overall morphology suggests a relatively evolved system, likely with a dominant stellar population. No major disturbances from mergers are visible, though the possibility of past minor interactions cannot be ruled out given slight asymmetries in the outer envelope. The galaxy seems to be relatively isolated in the observed field.
