The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The overall color profile appears relatively red, suggesting an older stellar population and potentially lower ongoing star formation activity. There is little evidence of spiral arms or a defined disk structure. The light distribution is fairly even, with no highly distinct features like bright knots of star formation or dust lanes readily apparent. The galaxy appears approximately round, without a strongly elongated or distorted shape, although there might be some indications of minor irregularities in its outer regions, potentially hinting at past interactions or mergers. The galaxy does not appear to be undergoing any significant merger events, but it might be showing some signs of minor disturbances.