The galaxy appears as a relatively smooth, elliptical structure. It exhibits a central concentration of light that gradually fades outwards. The galaxy's overall shape is somewhat round, though it does not seem perfectly spherical. There is no visible spiral structure, nor is there strong evidence of a prominent disk. Faint irregularities or minor disturbances are present, potentially indicating past interactions or mergers, though the dominant morphology appears largely undisturbed. The color is consistent with an older stellar population, trending towards the redder end of the spectrum, with some blue towards the core. There is no evidence of significant active star formation as indicated by a lack of bright blue star-forming regions or strong emission lines. The galaxy is a relatively isolated object, with no visually apparent major companions or nearby galaxies undergoing significant interaction. Overall, it presents as a relatively quiescent elliptical galaxy.
