The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It possesses a distinct cigar shape, suggesting a prolate spheroid structure. The galaxy displays a prominent central bulge, which gradually diffuses into a fainter, extended halo. Color gradients are subtle, with a slightly redder hue concentrated towards the core, potentially indicating an older stellar population dominating the central region. The overall color suggests a relatively low rate of ongoing star formation. There is no visual evidence of spiral arms, dust lanes, or other distinct features typically associated with spiral or irregular galaxies. No major tidal disturbances are apparent.
