The galaxy presents as a somewhat elongated, smooth object with a noticeable color gradient. The central region appears significantly brighter and exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Moving outward from the center, the color transitions towards a more reddish tone. There is little evidence of distinct spiral arms or prominent dust lanes. The overall structure appears relatively undisturbed, with no obvious signs of a major ongoing merger event, though subtle tidal features cannot be ruled out at this resolution. The elongation suggests an elliptical morphology, possibly of type E4-E6. The light distribution appears to be relatively even, with no significant clumpy features or regions of intense star formation readily apparent.
