This galaxy presents an elongated, somewhat fusiform morphology. The central region exhibits a concentration of light, appearing relatively smooth and more luminous than the outer regions. This central area displays a warm hue, potentially indicating an older stellar population or significant dust obscuration.

Moving outward from the core, the galaxy transitions to a bluer color profile. This could signify the presence of younger, hotter stars within a disc component. The light distribution in these outer regions is less uniform, exhibiting some subtle asymmetries or irregularities. There are hints of potential disturbances, such as faint, extended tidal features or warped disc structures, however these characteristics are not prominent. There is a subtle visual perturbation on the edges of the galaxy, but it does not appear to be a major disruption.

Overall, the galaxy appears to be an intermediate type, possibly a late-type spiral or lenticular galaxy experiencing some minor gravitational interaction.
