The galaxy presents a somewhat amorphous, diffuse appearance, with no readily discernible spiral arms or a prominent central bulge. The light distribution is relatively smooth, suggesting a possible elliptical or lenticular morphology, though some subtle features suggest a possible disk component. There's a slightly disturbed morphology, indicating a possible minor merger event. 

The color profile suggests a range of stellar populations, with a mix of older, redder stars and a component of younger, bluer stars. The lack of bright, concentrated star-forming regions suggests a relatively low star formation rate. The galaxy exhibits a moderate amount of internal extinction, possibly due to dust.
