The galaxy presents an elliptical morphology, with a smooth, featureless light distribution. Its shape is elongated, appearing cigar-shaped rather than perfectly round. The galaxy's color profile suggests a dominant population of older stars, evident from the reddish-yellow hue at its core. Fainter, bluer light is present towards the outer edges of the galaxy, which may indicate some regions of ongoing, albeit low, star formation. There is no clear evidence of a spiral structure, major mergers or significant tidal disturbances in this image. Overall, the galaxy appears to be a relatively quiescent system with a substantial stellar mass.
