The galaxy appears as a single, relatively smooth object. Its morphology suggests a spheroid shape, neither perfectly round nor highly elongated. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions, indicating a moderate level of central concentration. There's a slight hint of a disturbed structure, possibly from a minor interaction. The galaxy is slightly dimmer, and its colors are relatively uniform across its body, suggestive of an older stellar population with minimal ongoing star formation. There is a hint of possible merger activity, as the galaxy is elongated in one direction, and also appears to have some irregularities along its surface.
