The galaxy exhibits a generally smooth morphology, appearing as a slightly elongated, cigar-shaped structure. A central bulge region is visible, displaying a concentrated brightness. The overall color profile indicates a population of older stars, with a tendency towards redder hues throughout the main body of the galaxy. There is some indication of faint, bluer regions near the edges which may indicate some ongoing low-level star formation. No distinct spiral arms are clearly discernible, nor is there evidence of any major merger events or tidal disturbances. The structure looks relatively undisturbed.
