The galaxy exhibits an overall elliptical morphology, though subtle irregularities suggest a more complex structure. The light distribution appears relatively smooth, with a central concentration that gradually fades outwards. A slight elongation is visible, indicating a degree of flattening. The galaxy's color is predominantly yellowish-white, with hints of bluer tones in certain regions. This suggests a mix of stellar populations, with older stars contributing to the yellow hue and pockets of younger, hotter stars responsible for the blue. The lack of distinct spiral arms or a prominent disk implies that this galaxy is likely an elliptical galaxy. Evidence of potential tidal interactions or minor disturbances are noticeable, indicating possible past merger events. The galaxy has an estimated effective radius of approximately 8.3 kiloparsecs.
