The galaxy presents a generally smooth morphology, with a notable absence of defined spiral arms or significant irregularities. The shape is elongated, appearing somewhere between round and cigar-shaped. The central region exhibits a concentrated, bright bulge, suggesting a relatively old stellar population. There is some evidence of bluer light towards the outer regions, hinting at the presence of younger stars or ongoing star formation, although it appears to be at a low rate. The overall color of the galaxy indicates a mix of stellar ages, with the redder bulge contrasting with the bluer outer regions. There are no obvious signs of tidal disturbances or major mergers.
