The galaxy presents an overall elliptical morphology. The light distribution appears relatively smooth with a concentrated central region. There is a notable lack of distinct spiral arms or a well-defined disk structure. The overall shape appears moderately elliptical rather than perfectly spherical or highly elongated. There is a slight hint of possible minor disturbance or interaction, based on subtle irregularities in its outer regions. No obvious signs of an ongoing major merger event are observed. The dominant color appears to be a blue-green hue. This may indicate relatively active star formation, or a unique composition of stars.
