The galaxy presents as a moderately inclined, disk-like structure. Its central bulge appears substantial and exhibits a smooth, concentrated distribution of light, indicative of an older stellar population. The disk component is less defined but visible with tightly wound spiral arms that are close to the bulge. These arms are not well resolved, suggesting they are relatively smooth with few star forming regions. A slight colour gradient is visible. The inner region has a more yellow hue gradually shifting to blue, suggestive of active star formation in the outer spiral arms. The smooth texture of the light indicates that this is most likely a relatively evolved disk galaxy with characteristics intermediate between a spiral and a lenticular system. There is no obvious evidence of significant ongoing merger activity or tidal disturbances in the immediate vicinity.
