The galaxy appears to be a relatively compact, roughly elliptical or lenticular structure. It exhibits a bright, concentrated central bulge, suggesting a high density of stars in its core. There's a relatively smooth transition in brightness from the center outwards, with no sharply defined spiral arms or strong dust lanes visible in this image. The color profile suggests a generally bluer tint in the galaxy's core compared to the outer regions. Based on the overall morphology, the galaxy shows some evidence of disturbances, perhaps due to past or ongoing gravitational interactions. These disturbances appear as slight asymmetries or irregularities in the galaxy's overall structure, but are not readily visible in the image.
