The galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, suggesting a dense stellar population or possibly an active galactic nucleus. Moving outward from the core, the light intensity gradually decreases, with no distinct spiral arms or bar-like features readily apparent. There may be a hint of a diffuse halo surrounding the main body of the galaxy. Overall, the morphology is consistent with an evolved system, likely dominated by older stellar populations. No significant tidal features or signs of recent major mergers are immediately obvious, however, there is some minor disturbance. The galaxy has a generally rounded shape. The light distribution is slightly elongated.
