The galaxy presents a predominantly smooth morphology. It exhibits an elliptical shape, appearing elongated with a high degree of oblateness. The light distribution suggests a centrally concentrated structure, with the luminosity gradually decreasing towards the outer regions. There is a subtle color gradient, with the core exhibiting a slightly bluer hue compared to the more reddish outer halo. No distinct spiral arms or prominent dust lanes are discernible in the image, supporting the overall classification as a relatively undisturbed system. There is no clear evidence of recent or ongoing major mergers, though some minor disturbances cannot be entirely ruled out at this resolution. Overall, this galaxy appears to be a typical example of an early-type galaxy.