The galaxy exhibits a generally smooth morphology. It presents with a bright central bulge which gradually diffuses outwards into a slightly elongated form, indicating a moderate ellipticity. The color profile suggests a higher concentration of older stellar populations, as evidenced by the redder hues in the outer regions of the galaxy, in comparison to the inner regions. There is no apparent spiral structure, arm features or dust lanes, but a hint of blue coloration is present in the inner regions. There are no indications of any major merger events or significant tidal disturbances. The galaxy appears relatively isolated in this field.