The galaxy presents as a centrally concentrated object. Its overall form appears largely amorphous, exhibiting a generally smooth texture without well-defined spiral arms or a prominent bar structure. The central region is dominated by a bright, concentrated core, potentially indicative of an active galactic nucleus or a dense stellar population. 

The color profile of the galaxy displays a notable variation. The core shows a bluish hue, suggesting the presence of younger, hotter stars engaged in active star formation, or possibly the radiation from an AGN. Moving outward from the core, the galactic disk transitions to a redder color, hinting at an older stellar population. However, the light in the object is faint, as the object is distant.

There is no visible evidence of distinct tidal tails or shell structures usually associated with significant galaxy interactions or mergers, though some minor disturbances are indicated. The overall appearance seems relatively undisturbed.
