The galaxy appears as a relatively compact object with a roughly elliptical morphology. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus or bulge. There's a gradual decrease in luminosity moving outward from the core, transitioning from a yellow-orange hue at the center to a slightly bluer and fainter outer halo or disk. The color gradient suggests a possible difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outer regions. The overall smooth appearance with a lack of distinct spiral arms indicates a classification leaning towards an elliptical or lenticular galaxy type. There might be some minor disturbances or irregularities in the outer disk, possibly indicating a past or ongoing minor merger event, but the overall structure does not suggest a significant ongoing interaction or major disruption.
