The galaxy presents as a relatively smooth, elliptical-like structure. A slight elongation is apparent with an orientation of approximately 55 degrees. The central region exhibits a higher concentration of light, gradually decreasing in intensity towards the outer edges. There is a faint, diffuse halo surrounding the main body of the galaxy. The color profile appears to be dominated by reddish hues, suggesting a population of older stars, but there is some indication of bluer areas closer to the center. There are no distinct spiral arms, dust lanes, or other prominent features typically associated with spiral galaxies. Faint disturbances of the light profile may be present, but could possibly be due to noise. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy, possibly an elliptical or lenticular type.
