This galaxy presents an overall elliptical morphology, with a significantly higher concentration of light towards the center. The nucleus appears to be bright, suggesting a dense stellar population or possible AGN activity, though further spectral analysis would be required to confirm this. The galaxy exhibits a smooth light distribution, with no apparent spiral arms or distinct dust lanes. The ellipticity suggests a non-negligible angular momentum, possibly indicative of a past minor merger event, although the overall structure appears largely undisturbed. Color gradients are subtle, with a slight reddening toward the central region. The size is moderate, consistent with a typical elliptical galaxy at its estimated distance. It appears to be a relatively passive system with low levels of on-going star formation.
