The observed galaxy presents a relatively compact morphology with a noticeable central bulge. The galaxy exhibits an overall smooth appearance, with minimal evidence of spiral arm structure. The bulge region appears to be dominant within the galaxy's structure, indicating a higher concentration of older stellar populations. Faint, diffuse emission is observed extending outwards from the central region, possibly indicative of a weak disk component or tidal debris.

There is some evidence of minor asymmetry in the outer regions of the galaxy, potentially suggesting a recent interaction or minor merger event. The overall color is slightly redder than expected, possibly indicative of a relatively high redshift, or dust extinction. The compact morphology and high central concentration suggest a classification as an early-type galaxy.
