The galaxy exhibits a relatively smooth morphology, with an intermediate degree of roundness. The primary color components appear to be dominated by redder hues, shifting towards yellow and white at the core and inner regions. There is evidence of a possible disk structure, but overall it gives the impression of a smooth, potentially spheroid structure.

There is some indication of minor disturbances in the galaxy's structure, but no clear sign of ongoing major merger events. The galaxy does not appear to be completely symmetrical, and it shows areas that are less uniform than other regions, which are relatively smooth. The galaxy size appears compact, with a visible diameter estimated around 6 kiloparsecs. Based on the observed colors, stellar mass is expected to be fairly high and star formation rate is predicted to be relatively low. 
