The galaxy presents as a largely smooth, elliptical morphology. There is little evidence of spiral arm structure or significant disk component. The galaxy exhibits a concentrated central bulge that appears more luminous than its surrounding regions. The color profile indicates that the galaxy may be dominated by an older stellar population, exhibiting a yellowish hue. There are no prominent dust lanes or significant tidal disturbances visible, suggesting it is a relatively undisturbed system. The isophotes appear to be elongated, more "in between" round and cigar-shaped. There is no evidence of a strong active galactic nucleus based on the information and lack of any obvious jet features.
