The galaxy presents as a somewhat elliptical structure with a relatively smooth, centralized luminosity profile. There is a bright, concentrated core exhibiting a slightly bluer color than the outer regions. The galaxy lacks any prominent spiral arm structures or distinct morphological features, suggesting a more spheroid-dominated or elliptical classification. The overall color index indicates a potential mix of stellar populations, with the bluer core hinting at ongoing or recent star formation activity, while the more red-shifted outer regions might contain older stellar populations. There might be some minor disturbance happening within the galaxy, but it appears to be quite smooth.
