The galaxy presents as an elliptical morphology, elongated in shape. A smooth distribution of light is observed throughout its main body, with a concentration of luminous intensity towards the core. The color profile displays a redder hue, suggesting a dominant population of older stars. Subtle tidal features or minor disturbances may be present, but not significantly pronounced, indicating the potential for past interactions but no strong ongoing merger activity. An estimate of its size places it around 5 kiloparsecs in radius. The overall structure appears consistent with an evolved system exhibiting relatively low star formation rates.
