The observed galaxy presents a morphology intermediate between elliptical and spiral types, showing characteristics of both. The central region displays a bright, concentrated bulge, indicative of a substantial population of older stars. This central luminosity decreases gradually with increasing radius.

A faint, diffuse disk-like structure extends outward from the bulge. Within this disk, there are some faint, diffuse, blue-ish regions, suggesting the presence of younger stars and possible ongoing star formation. However, distinct spiral arm structures are not readily apparent.

The overall shape suggests the galaxy is viewed at a slight angle, but it's difficult to determine the exact inclination. Irregularities are observed in the outer regions of the disk. These could be the result of a minor merger event or tidal interaction, as the galaxy's shape is slightly distorted. There may be faint tidal features or streams extending beyond the main body of the galaxy, though more detailed observations would be needed to confirm this.
