The galaxy presents as a somewhat elongated, cigar-shaped structure with a smooth, featureless appearance. There is a subtle color gradient visible, with a slightly bluer hue towards the central regions and a gradual shift to redder tones in the outer areas. This color variation suggests a possible distribution of stellar populations, with younger, bluer stars concentrated towards the center and older, redder stars more prevalent in the outer regions. There is no apparent spiral arm structure or evidence of ongoing star formation visible. The galaxy's morphology indicates a relatively evolved system, potentially consistent with an elliptical galaxy. The lack of significant disturbances suggests it is not undergoing any major interactions with other galaxies.
