The galaxy appears as an elliptical-like structure, characterized by a smooth, diffuse light distribution. There is little evidence of spiral arms or distinct features within the galaxy's body. The galaxy exhibits a fairly regular, rounded morphology, but is not perfectly spherical. The color profile indicates a general yellowish hue, suggestive of an older stellar population and a lack of ongoing, significant star formation activity. The galaxy's core shows a slightly brighter intensity than the surrounding regions, possibly indicating a central concentration of stars. Although its overall appearance is generally undisturbed, there may be a hint of slight asymmetry or irregularity, suggesting a past interaction or minor perturbation, however, it does not appear to be undergoing a major merger or significant tidal disruption.
