The galaxy exhibits a relatively smooth morphology, with a concentrated central bulge that appears to be the brightest region. There is little evidence of distinct spiral arm structures; rather, the light distribution suggests an elliptical or lenticular galaxy type. The overall color of the galaxy is yellowish-orange, indicative of a population of older stars with low star formation. No major disturbances or merging events are clearly visible in the galaxy's structure. The galaxy appears somewhat rounded in shape, suggesting that it is being viewed from a closer-to-face-on angle. There are no bright blue star-forming regions that can be easily seen, which would suggest that star formation is largely suppressed.