The galaxy presents as an elliptical or lenticular type, displaying a smooth, featureless morphology with no discernible spiral arms or bar structure. Its overall shape is predominantly round, with a slight elongation. The light distribution is concentrated towards the center, indicating a prominent bulge. The core exhibits a bright, yellowish hue, suggesting an older stellar population. The galaxy's outer regions fade gradually, exhibiting a redder color, which may be due to a higher proportion of older, cooler stars or dust obscuration. There is no apparent evidence of ongoing star formation. No tidal tails or other signs of recent merger activity are visible. The galaxy appears to be a relatively isolated system, undisturbed by interactions with neighboring galaxies.
