The galaxy exhibits an elongated, cigar-like morphology. A prominent bulge is observable, with light distribution concentrated toward the center, indicating a significant population of older stars. The galaxy shows a smooth appearance. There may be some faint disk-like features extending outwards from the bulge, these are embedded within a more diffuse halo.

Based on the color gradients, the inner regions of the galaxy appear more yellowish, while the outer edges exhibit a slightly bluer hue, suggesting the presence of younger stars. However, the low specific star formation rate suggests a lack of star formation. The galaxy shows no signs of major disturbances.
