The galaxy presents a generally smooth morphology with a central bulge that appears to be a yellowish hue. Surrounding the central region is a slightly less concentrated area of light, with a hint of blueish tint on one side, suggesting the possibility of localized star formation activity within that region. The galaxy appears somewhat elongated rather than perfectly circular and has possible signs of distortion. Overall, the galaxy seems to be in a relatively mature stage of its evolution with a fair number of old stars. There may be minor disturbances in the distribution of its light, indicating the possibility of interactions or minor mergers in its past.
