This galaxy exhibits a generally smooth morphology with a bright central bulge that appears somewhat rounded. There is some evidence of possible features such as a disk, or the beginnings of spiral arms. The galaxy's shape ranges from round to cigar shaped, with the greatest portion being in between. The color profile transitions from the yellowish hue of the core to reddish tones in the outer regions, suggesting varying stellar populations or dust distribution. There appears to be at least one minor disturbance, possibly an interaction with a smaller object, or gravitational distortion. There is no strong evidence of an ongoing major merger.