The object presents as a galaxy exhibiting a slightly elongated morphology, appearing somewhat cigar-shaped. A concentrated central bulge is visible, indicating a significant concentration of older stellar populations, contributing to its smooth appearance and reddish-yellow hue. The galaxy displays a non-negligible disk component, although the disk lacks clearly defined spiral arms and appears relatively smooth. There are no obvious signs of ongoing major merger activity, though a slight asymmetry or minor disturbance is hinted in its structure. The colour profile indicates that star formation is relatively subdued, contributing to a dominant population of older, redder stars. Overall, the galaxy's morphology and colour suggest it is an intermediate-mass system approaching the red sequence.
