The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology without prominent spiral arms. The light distribution appears concentrated towards the center, suggesting the presence of a central bulge. The galaxy appears elongated, with a noticeable disk component. There is some evidence of minor disturbances or interactions, possibly in the form of tidal features or asymmetries in the outer regions, but it does not seem to be undergoing a major merger event. Stellar formation is present, but not pronounced. The color gradient suggests a mixed stellar population, with older, redder stars concentrated in the bulge and a younger, bluer population present in the disk. 
