The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth morphology without prominent spiral arms or a well-defined disk. The light distribution is centrally concentrated, fading gradually outwards. There is a slightly elongated shape, but it leans toward round more than oblong. Evidence of a potential minor interaction or merger exists, with some subtle irregularities or faint tidal features. The colors are generally consistent with an older stellar population, with a modest degree of ongoing star formation.
