The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a high degree of smoothness with a concentration of light, suggesting a substantial spheroidal component, possibly a bulge. The color profile transitions from a warmer, yellowish core to cooler, bluer hues in the outer regions, indicative of differing stellar populations and/or dust distribution. The pronounced ellipticity implies a significant amount of ordered motion within the system or a past merger event. There is no apparent spiral arm structure or bar feature visible in this observation, suggesting this is likely an elliptical galaxy with relatively low star formation. There may be some minor disturbances or tidal features that are barely visible which could indicate it experienced a minor merger.