This galaxy presents as a relatively smooth, elliptical-shaped object. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or potentially an active galactic nucleus. Moving outwards from the core, the light appears to gradually diminish, indicating a decreasing stellar density. There is a subtle colour gradient, with the central region appearing slightly yellower than the outer edges, possibly indicative of an older stellar population in the core. The galaxy displays a mild elongation, deviating slightly from a perfectly circular form, tending toward a cigar shape. There is no clear evidence of spiral arms, dust lanes, or significant tidal disturbances, suggesting a relatively quiescent and evolved system. The galaxy appears to be well-isolated, showing no signs of interaction with other galaxies in its immediate vicinity. The overall appearance suggests a mature elliptical galaxy with ongoing, but relatively low, star formation.
