The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that transitions smoothly outwards to a fainter, diffuse halo. There is no discernible spiral structure or significant dust lanes visible in this image. The galaxy's color profile suggests a population of older stars, indicated by the relatively redder hues. There is little evidence of ongoing major star formation activity within the galaxy, aligning with its smooth, bulge-dominated morphology. The object exhibits a moderately elongated shape. Close inspection reveals subtle, minor disturbances or asymmetries, possibly indicating a past interaction or minor merging event, but this is not a strong feature. Overall, the galaxy presents as a fairly undisturbed, evolved system.
