The galaxy presents a morphology indicative of an elliptical type. Its overall form is relatively smooth and centrally concentrated, with a notable lack of distinct spiral arms or a prominent disk-like structure. The color profile leans towards the redder end of the spectrum, suggesting a population of older, cooler stars. This redder hue implies that star formation activity is likely subdued. The galaxy exhibits an intermediate apparent roundness; it is neither perfectly spherical nor highly elongated. There are no obvious signs of ongoing or recent major merger events. There might be a subtle indication of a minor disturbance in its structure, but it is subtle. The galaxy's size appears moderate. Overall, this galaxy appears to be a relatively quiescent, evolved system.
