The object presents as a slightly elongated galaxy with a bright, concentrated central bulge region. The galaxy exhibits a relatively smooth overall appearance with minimal discernible spiral arm structure or distinct features extending outward from the central region. The light distribution suggests the majority of the luminosity originates from the core, indicative of either an active galactic nucleus or a dense stellar population. The outer regions of the galaxy appear faint and diffuse, with a blueish hue dominating the color profile. There is some slight visual distortion, suggesting possible gravitational interactions.
