The galaxy presents as an elongated, cigar-shaped structure with a smooth, featureless appearance. Its color is primarily a blend of blue and white, suggesting a mixture of stellar populations. The core of the galaxy exhibits a brighter, more concentrated region, indicating a possible central bulge. There is no visible spiral arm structure or dust lane obscuration apparent in this image, supporting the conclusion that it may be an elliptical type galaxy. The overall uniformity and lack of distinct features within the galaxy body further suggest a relatively quiescent star formation rate. There is no evidence of any significant merging activity or tidal disruption, based on its regular morphology. The galaxy is estimated to be several kiloparsecs in radius.
