The galaxy presents a somewhat elliptical morphology, with a smooth, centrally concentrated light distribution. There is evidence of a slight distortion, possibly indicative of a minor disturbance or interaction. The galaxy's color appears relatively red, suggesting a population of older stars and a lower rate of ongoing star formation. The main body of the galaxy is elongated, with a suggestion of a bar-like feature running through its core. There is a hint of a disk or spiral arm structure, but it appears faint and ill-defined. Overall, this galaxy appears to be in a transitional phase, possibly evolving from a spiral to an elliptical type, with characteristics suggesting a system that has experienced, or is currently experiencing, some form of gravitational interaction.
