This galaxy exhibits a generally smooth, elliptical morphology. The core region appears highly concentrated, with a bright, yellowish hue suggesting an older stellar population. There is a lack of discernible spiral arm structure or dust lanes within the galaxy's body. A faint, extended halo is present around the central bulge, gradually fading into the background sky. The galaxy's overall shape is predominantly round, with a slight deviation towards a cigar shape. The absence of major disturbances implies no recent merger events. The galaxy appears as an isolated system. The color suggests that there is a very low amount of star formation within the galaxy.
