The galaxy presents an overall elliptical morphology, appearing elongated with a high degree of axis ratio. Its light distribution appears relatively smooth and centrally concentrated, indicative of an evolved stellar population. The central region exhibits a yellowish hue, potentially due to a higher concentration of older, redder stars. There is no clear spiral arm structure visible. The galaxy does not appear to be undergoing any major merging events. The faint outer regions transition gradually from the brighter core, suggesting a smooth density profile.
