The galaxy appears as a centrally concentrated object with a smooth morphology. It exhibits a roughly elliptical shape, tending towards a more circular form. There is a high degree of central concentration of light, with a gradual falloff in brightness towards the outer regions. The light distribution is largely uniform and lacking in defined spiral arms or distinct features indicative of active star formation regions. The galaxy is of intermediate color, with a slight reddish hue, suggestive of a population of older stars. There are some subtle signs of interaction or minor disturbance. No strong evidence of a recent or ongoing major merger is apparent. 
