The galaxy presents a largely smooth morphology, with a dominant central bulge. The overall shape approximates a spheroid, displaying significant rotational symmetry. There may be a hint of a disk component, but it is not well-defined or prominent. There is no apparent evidence of recent or ongoing major merger activity. The color profile suggests a population of older stars, possibly with limited ongoing star formation. A minor asymmetry is noted in the shape, though it is difficult to tell whether that is a sign of an interaction with a smaller body, or merely some kind of visual artifact. Overall, the galaxy appears to be a relatively evolved system.
