The galaxy presents as an elliptical morphology. Its core exhibits a concentrated, luminous yellowish-white intensity, indicative of an older stellar population. The galaxy is surrounded by a less concentrated halo. There's a hint of a faint, blue disk-like structure that is angled along the horizontal axis, though the resolution makes it difficult to discern distinct spiral arms. There are notable color variations in the surrounding halo, with some regions exhibiting bluer tones, suggesting the presence of younger stars or active star formation in these areas. Other areas show patches of redder hues which are likely older stellar populations. There's some indication of possible tidal features, but the image quality doesn't allow for a definitive identification. The overall structure hints at a potential merger history or ongoing interaction with a companion.
