The galaxy exhibits a roughly elliptical morphology, though with some irregularities in its overall structure. The central region of the galaxy appears bright and relatively uniform in color, suggesting a dominant population of older stars or significant dust obscuration. A subtle disk structure appears to surround the nucleus. This disk appears to be more complex, showing some level of disturbance, most likely a minor disturbance rather than a major merger. Redder hues in the outer regions may indicate a population of older stars or dustier regions within the disk. There are also hints of some bluer color closer to the center of the galaxy which could indicate star formation, though this is not uniform throughout the galaxy. Overall, the galaxy appears to be in an isolated environment, with no strong indications of a major ongoing merger.
