The galaxy presents a flattened, elliptical morphology, appearing elongated in shape, specifically cigar-shaped. There is a smooth light distribution across the galaxy. The central region exhibits a concentrated brightness with an orange hue, which may indicate an older stellar population and reduced star formation in this area. Fainter, bluer outskirts suggest the presence of a younger stellar population and ongoing star formation, although this is not very pronounced. No distinct spiral arm structure is visible. There is no obvious evidence of a major merger or significant tidal disturbance. There might be a minor interaction occurring, but the structure is generally undisturbed. Overall, it is a lenticular or elliptical galaxy with a relatively smooth appearance.
