The galaxy appears to be an elliptical type, characterized by a smooth, featureless light distribution. It exhibits a somewhat elongated, cigar-shaped morphology, with a bright, concentrated central region likely indicating a significant stellar density. There is no apparent spiral arm structure or dust lane obscuration evident in the image. The color profile suggests a relatively old stellar population, with a subtle reddish hue. The object does not appear to be undergoing any major merger events or significant tidal disturbances.
