The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a higher density of older stellar populations. Moving outwards from the core, the light appears to gradually diminish, transitioning into a more diffuse halo. There is a subtle color gradient visible, with the core appearing slightly redder in contrast to the more greenish surrounding areas. No prominent spiral arms or distinct dust lanes are discernible, supporting the smooth classification. There is no strong evidence of major mergers or significant tidal disturbances within the galaxy's immediate structure. The galaxy has an overall elliptical shape, with an axis ratio that shows it is somewhat elongated, but not cigar-shaped.
