The galaxy presents as a relatively smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, fading gradually into the outer regions. There is a slight elongation visible, suggesting an oblate spheroid shape rather than a perfect sphere. No distinct spiral arms or other features of a disk galaxy are discernible. The overall color appears to be leaning towards a redder hue. There is no evidence of significant ongoing star formation based on the lack of blue colors and absence of distinct HII regions. The galaxy appears relatively undisturbed, showing no obvious signs of recent merger activity or tidal interactions. The smooth and featureless nature suggests this is likely an older galaxy composed primarily of older stellar populations.
