The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless light distribution. The central region shows a high concentration of light, gradually decreasing towards the edges. The color profile indicates a redder core, possibly due to an older stellar population. A faint blue tinge is visible in the outer regions, potentially suggesting the presence of younger stars or low-level star formation. The overall shape is more lenticular, leaning towards a cigar shape, with no apparent spiral arm structures or dust lanes visible. There is no obvious evidence of any major ongoing merger activity, though minor tidal disturbances may be present.
