The galaxy appears to be a relatively smooth, elongated object. Its overall shape is reminiscent of a cigar or spindle, lacking a prominent disk or spiral arms. The light distribution is concentrated towards the center, gradually fading towards the edges. There is a hint of a redder hue towards the center, possibly indicating an older stellar population or a concentration of dust. No significant morphological disturbances or interactions with neighboring galaxies are readily apparent. The galaxy appears to be a relatively isolated system. The general lack of blue light suggests that the galaxy is not undergoing intense star formation. Overall, the galaxy seems to be an elliptical galaxy.
