The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. A distinct bulge is observable at the galaxy's core, displaying a yellow-white hue, suggesting an older stellar population. A faint, diffuse halo surrounds the central bulge, fading gradually into the background. The halo appears largely smooth, with no obvious spiral arm structure. To the right of the main galaxy, there is a region of bluer light, indicating a potentially younger stellar population or ongoing star formation. This area seems to be causing some sort of disturbance.
