The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with the light intensity decreasing gradually from the core outwards. There is little evidence of spiral arm structure or distinct features that would classify it as a spiral galaxy. The overall shape appears somewhat elongated but with the 'Round Fraction' relatively low.

The color distribution suggests a population dominated by older stars, with a subtle reddish tint, especially in the outer regions. There are hints of blue, potentially indicating a degree of ongoing star formation, likely minimal and confined towards the central regions.

There might be very minor disturbances to the galaxy's shape, possibly due to a past interaction or merger, but the overall structure remains relatively undisturbed. The galaxy appears to be relatively isolated based on the image, with no obvious signs of a major ongoing merger.
