The object appears to be an edge-on spiral or lenticular galaxy exhibiting a distinct central bulge that transitions into a relatively smooth disk structure. The bulge displays a yellowish hue, possibly indicative of an older stellar population. The disk appears bluer, suggesting the presence of younger stars and star formation regions, although this is somewhat subdued. The shape of the galaxy is elongated, almost cigar-shaped. There's no prominent evidence of strong tidal interactions or a recent major merger event, though there might be some minor disturbances in the outer regions of the disk. The galaxy appears relatively isolated in this field.
