This galaxy appears to be relatively compact, exhibiting a bright central region surrounded by a fainter, more diffuse halo. The central region displays a yellow-white hue, potentially indicative of an older stellar population, while the surrounding halo shows hints of blue, suggesting the presence of younger, hotter stars.

The morphology is somewhat disturbed, with the presence of a plume-like structure extending outwards from the main body of the galaxy. This could indicate a tidal tail resulting from a past gravitational interaction, or it could potentially be a remnant of an ongoing merger event.

Overall, the galaxy presents characteristics of both an elliptical galaxy, due to its compact shape and bright central region, and an irregular galaxy, due to the observed disturbance and asymmetric features. Further spectroscopic analysis would be beneficial to ascertain the redshift, stellar population distributions, and any potential signs of active galactic nuclei.
