The galaxy presents a smooth, elliptical morphology. It appears somewhat elongated, deviating from a perfectly circular shape, suggestive of a cigar-like form. The central region exhibits a concentrated brightness, indicating a prominent nucleus. A gradual decrease in luminosity is observed moving outwards from the core. There is little evidence of strong spiral arms or dust lanes. The overall color profile suggests an older stellar population. The galaxy does not appear to be undergoing any major merging events or tidal disturbances based on the image, though there is a hint of some minor disturbance, given that the galaxy is not perfectly smooth.
