The galaxy presents as a relatively small, yet distinct, celestial object. Its morphology is largely dominated by a smooth, somewhat amorphous structure. There is a subtle elongation of the main body along a horizontal axis, suggesting a possible disklike component seen nearly edge-on, however, no definitive spiral arm structures are visible within the resolution. The central region exhibits a bright, concentrated core, indicative of a possible active galactic nucleus or a dense stellar population. Faint tidal features or disturbances are hinted at but are not well-defined. Overall color is weighted slightly towards redder wavelengths, with the brightest regions appearing blue-green, suggestive of possible star forming regions. There is a potential indication of a minor interaction or merger event, as hinted at by the potential faint tidal features, but further study is required to ascertain the nature of this system.
