The galaxy presents an elliptical morphology, with a smooth and largely featureless appearance, exhibiting a slight elongation. The color profile indicates a dominant population of older stars, contributing to the observed redder hues. There is a central concentration of light suggesting the presence of a galactic bulge. There appears to be no prominent disk structure or spiral arm features visible in this image. The galaxy exhibits a consistent light profile, with no signs of major disturbances, such as tidal tails or other indicators of recent merger events.
