The galaxy presents as a single, relatively smooth and rounded entity. A dominant central bulge exhibits a concentrated, bright yellowish hue, likely indicating an older stellar population. The galaxy's overall color profile suggests a population dominated by older, redder stars, with minimal evidence of ongoing, active star formation. There is a subtle hint of a disk structure, but the image resolution and galaxy's presentation preclude detailed analysis of any spiral arms or bars. Minor disturbances within the galaxy, such as tidal tails or interacting companion galaxies, are not evident. The morphology appears largely undisturbed, indicating a relatively quiescent evolutionary state.
