The galaxy presents a generally smooth morphology, appearing as a concentrated central bulge surrounded by a fainter, more diffuse halo. The color is predominantly a warm, yellowish hue, suggesting an older stellar population with fewer young, hot stars. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy exhibits a roughly elliptical shape, although not perfectly circular. Subtle irregularities in the outer halo might hint at past minor interactions or disturbances. The overall appearance suggests an evolved system with a relatively low rate of recent star formation.
