The galaxy appears to be an elliptical type, characterized by a smooth and centrally concentrated light distribution. Its shape is generally spheroidal, showing a lack of distinct spiral arms or a well-defined disk. There is an absence of significant dust lanes. The galaxy's color is generally redder, which would indicate an older stellar population, consistent with elliptical galaxies. There is some evidence of minor disturbances or interactions, as subtle asymmetries and faint tidal features may be present in the outer regions, though these are difficult to discern clearly. The central bulge region exhibits high luminosity, indicating a dense concentration of stars in this area. The galaxy's profile fades gradually into the background, with no sharp edges or clear boundaries visible.
