The galaxy presents as a centrally concentrated, smooth object. The light profile appears diffuse, with a radial gradient decreasing from the center outwards. The core exhibits a yellowish hue, which may indicate an older stellar population and/or dust extinction. There is a subtle transition to redder hues within the galaxy’s outer regions. There are no visible spiral arms or prominent features indicative of active star formation that stand out. The roundness of the galaxy indicates a lack of a well-defined disk structure. The overall morphology suggests a galaxy that is relatively evolved. There is no evidence of a major merger event or tidal disturbances.
