This galaxy exhibits a primarily smooth morphology, appearing elliptical in shape when viewed from our vantage point. There is no defined spiral arm structure visible. The central region of the galaxy appears to be brighter, exhibiting a blue-white hue, suggesting a concentration of younger, hotter stars or a potential active galactic nucleus.

The galaxy’s outer regions show a more diffuse and reddish color, indicative of an older stellar population. There is a faint disk-like structure that is oriented almost edge-on to our line of sight, as indicated by the reddened edges. This could indicate the beginnings of star formation, which would correlate with the blue hue of the galaxy's center. The galaxy does not show any clear signs of significant tidal disturbances or ongoing mergers, however there is some irregular morphology.
