The galaxy presents an elongated, cigar-shaped morphology. The central region appears relatively smooth and bright, exhibiting a concentrated luminosity profile. This core is surrounded by a more diffuse, fainter halo or envelope of stellar material. There is no clear evidence of spiral arm structure. Instead, the light distribution suggests a spheroid-dominated system.

The color gradient suggests a relatively homogenous stellar population with no prominent regions of intense star formation visible in the image. The galaxy displays a blue hue throughout, and the overall appearance is relatively undisturbed, with only minor signs of any gravitational interactions or mergers.
