The galaxy presents as an elliptical or lenticular morphology, with a smooth, featureless light distribution. The central region exhibits a higher surface brightness, gradually decreasing towards the outer edges. The overall shape is elongated, approximately cigar-shaped, but significantly more rounded. There is no visible spiral arm structure or evidence of active star formation regions. The color profile suggests a population dominated by older stars. The galaxy shows no signs of a major ongoing merger event, though minor disturbances cannot be ruled out at this resolution.
